Exemplo n.º 1
0
def filterlocal(ui, vi, m, falloff, myid, main_node, number_of_proc):

    if myid == main_node:

        nx = vi.get_xsize()
        ny = vi.get_ysize()
        nz = vi.get_zsize()
        #  Round all resolution numbers to two digits
        for x in range(nx):
            for y in range(ny):
                for z in range(nz):
                    ui.set_value_at_fast(x, y, z, round(ui.get_value_at(x, y, z), 2))
        dis = [nx, ny, nz]
    else:
        falloff = 0.0
        radius = 0
        dis = [0, 0, 0]
    falloff = sp_utilities.bcast_number_to_all(falloff, main_node)
    dis = sp_utilities.bcast_list_to_all(dis, myid, source_node=main_node)

    if myid != main_node:
        nx = int(dis[0])
        ny = int(dis[1])
        nz = int(dis[2])

        vi = sp_utilities.model_blank(nx, ny, nz)
        ui = sp_utilities.model_blank(nx, ny, nz)

    sp_utilities.bcast_EMData_to_all(vi, myid, main_node)
    sp_utilities.bcast_EMData_to_all(ui, myid, main_node)

    sp_fundamentals.fftip(vi)  #  volume to be filtered

    st = EMAN2_cppwrap.Util.infomask(ui, m, True)

    filteredvol = sp_utilities.model_blank(nx, ny, nz)
    cutoff = max(st[2] - 0.01, 0.0)
    while cutoff < st[3]:
        cutoff = round(cutoff + 0.01, 2)
        # if(myid == main_node):  print  cutoff,st
        pt = EMAN2_cppwrap.Util.infomask(
            sp_morphology.threshold_outside(ui, cutoff - 0.00501, cutoff + 0.005),
            m,
            True,
        )  # Ideally, one would want to check only slices in question...
        if pt[0] != 0.0:
            # print cutoff,pt[0]
            vovo = sp_fundamentals.fft(filt_tanl(vi, cutoff, falloff))
            for z in range(myid, nz, number_of_proc):
                for x in range(nx):
                    for y in range(ny):
                        if m.get_value_at(x, y, z) > 0.5:
                            if round(ui.get_value_at(x, y, z), 2) == cutoff:
                                filteredvol.set_value_at_fast(
                                    x, y, z, vovo.get_value_at(x, y, z)
                                )

    mpi.mpi_barrier(mpi.MPI_COMM_WORLD)
    sp_utilities.reduce_EMData_to_root(filteredvol, myid, main_node, mpi.MPI_COMM_WORLD)
    return filteredvol
Exemplo n.º 2
0
def prgq(volft, kb, nx, delta, ref_a, sym, MPI=False):
    """
	  Generate set of projections based on even angles
	  The command returns list of ffts of projections
	"""
    from sp_projection import prep_vol, prgs
    from sp_applications import MPI_start_end
    from sp_utilities import even_angles, model_blank
    from sp_fundamentals import fft
    # generate list of Eulerian angles for reference projections
    #  phi, theta, psi
    mode = "F"
    ref_angles = even_angles(delta,
                             symmetry=sym,
                             method=ref_a,
                             phiEqpsi="Minus")
    cnx = nx // 2 + 1
    cny = nx // 2 + 1
    num_ref = len(ref_angles)

    if MPI:
        from mpi import mpi_comm_rank, mpi_comm_size, MPI_COMM_WORLD
        myid = mpi_comm_rank(MPI_COMM_WORLD)
        ncpu = mpi_comm_size(MPI_COMM_WORLD)
    else:
        ncpu = 1
        myid = 0
    from sp_applications import MPI_start_end
    ref_start, ref_end = MPI_start_end(num_ref, ncpu, myid)

    prjref = [
    ]  # list of (image objects) reference projections in Fourier representation

    for i in range(num_ref):
        prjref.append(model_blank(
            nx,
            nx))  # I am not sure why is that necessary, why not put None's??

    for i in range(ref_start, ref_end):
        prjref[i] = prgs(
            volft, kb,
            [ref_angles[i][0], ref_angles[i][1], ref_angles[i][2], 0.0, 0.0])

    if MPI:
        from sp_utilities import bcast_EMData_to_all
        for i in range(num_ref):
            for j in range(ncpu):
                ref_start, ref_end = MPI_start_end(num_ref, ncpu, j)
                if i >= ref_start and i < ref_end: rootid = j
            bcast_EMData_to_all(prjref[i], myid, rootid)

    for i in range(len(ref_angles)):
        prjref[i].set_attr_dict({
            "phi": ref_angles[i][0],
            "theta": ref_angles[i][1],
            "psi": ref_angles[i][2]
        })

    return prjref
Exemplo n.º 3
0
def plot_angles(agls, nx=256):
    from math import cos, sin, fmod, pi, radians
    from sp_utilities import model_blank

    # var
    im = model_blank(nx, nx)
    """
	c  = 2
	kc = 10
	# draw reperes
	for i in xrange(nx):
		im.set_value_at(i, int(nx / 2.0), 0.006)
		im.set_value_at(int(nx / 2.0), i, 0.006)

	# draw the circles
	lth = range(0, 90, kc)
	lth.append(90)

	for th in lth:

		if th == 90: color = 0.03
		else:        color = 0.006

		rc  = sin((float(th) / 180.0) * pi)
		rc *= (nx - 1)
		
		for n in xrange(3600):
			a  = (n / 1800.0) * pi
			px = nx / 2.0 + (rc - 1) / 2.0 * cos(a)
			py = nx / 2.0 + (rc - 1) / 2.0 * sin(a)
			im.set_value_at(int(px), int(py), color)
	"""
    # for each angles plot on circle area
    # agsl: [phi, theta, psi]
    ri = nx // 2
    rr = ri - 1
    conv = pi / 180.0
    for i in range(len(agls)):
        if agls[i][1] > 90.0:
            agls[i][0] = agls[i][0] + 180.0
            agls[i][1] = 180.0 - float(agls[i][1])

        rc = rr * sin(radians(agls[i][1]))
        rd = radians(agls[i][0])
        px = ri + rc * cos(rd)
        py = ri + rc * sin(rd)

        px = min(max(int(px + 0.5), 0), nx - 1)

        py = min(max(int(py + 0.5), 0), nx - 1)

        im.set_value_at(px, py, 1.0 + im.get_value_at(px, py))

    return im
Exemplo n.º 4
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def makeAngRes(freqvol, nx, ny, nz, pxSize, freq_to_real=True):
    outAngResVol = sp_utilities.model_blank(nx, ny, nz)
    data_in = freqvol.get_3dview()
    data_out = outAngResVol.get_3dview()

    if freq_to_real:
        mask = data_in > 0.0
    else:
        mask = data_in > 0.0
    data_out[mask] = pxSize / data_in[mask]

    return outAngResVol
Exemplo n.º 5
0
def montage2(inputstack, ncol, marginwidth=0, bkgd=0, outfile=None):
    """
	Generates montage of images into one image.
	Adapted from sxmontage.py
	
	Arguments:
		inputstack : Stack of input images to merge into montage
		ncol : Number of images per row
		marginwidth : Margin width, pixels
		bkgd : Background value of montage
		outfile : Optional output file with montage output
	Returns:
		montage : EMData object of image montage
	"""

    if isinstance(inputstack, str): inputstack = EMData.read_images(inputstack)

    # Get single-image dimensions
    nx = inputstack[0].get_xsize()
    ny = inputstack[0].get_ysize()

    # Get number of images and calculate montage dimensions
    numimgs = len(inputstack)
    numrows = (numimgs - 1) / ncol + 1

    # Create blank image
    montage_xdim = (nx + marginwidth) * ncol
    montage_ydim = (ny + marginwidth) * numrows
    montage = model_blank(montage_xdim, montage_ydim, 1, bkgd)

    # Loop through images
    for imgnum in range(numimgs):
        # Horizontal grid position is image# modulo NCOL
        colnum = imgnum % ncol

        # Montage is numbered from the top down
        rownum = numrows - 1 - imgnum / ncol

        xoffset = colnum * (nx + marginwidth)
        yoffset = rownum * (ny + marginwidth)
        insert_image(inputstack[imgnum], montage, xoffset, yoffset)

    if outfile: montage.write_image(outfile)

    return montage
Exemplo n.º 6
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    def test_input_image_returns_values_freq_to_real(self):
        nx = 10
        ny = 10
        nz = 10
        apix = 2
        test_data = numpy.arange(nx * ny * nz, dtype=numpy.float32).reshape(
            nx, ny, nz
        ) / (2 * nx * ny * nz)
        mask = test_data > 0

        blank_data = sp_utilities.model_blank(nx, ny, nz)
        data_in = blank_data.get_3dview()
        data_in[...] = copy.deepcopy(test_data)
        returned_data = sp_locres.makeAngRes(blank_data, nx, ny, nz, apix)

        expected_data = copy.deepcopy(test_data)
        expected_data[mask] = apix / test_data[mask]
        assert numpy.array_equal(expected_data, returned_data.get_3dview())
Exemplo n.º 7
0
    def test_input_image_returns_values_real_to_freq(self):
        nx = 10
        ny = 10
        nz = 10
        apix = 2
        test_data = numpy.arange(nx * ny * nz, dtype=numpy.float32).reshape(nx, ny, nz)
        mask = test_data >= 2 * apix

        blank_data = sp_utilities.model_blank(nx, ny, nz)
        data_in = blank_data.get_3dview()
        data_in[...] = copy.deepcopy(test_data)
        returned_data = sp_locres.makeAngRes(blank_data, nx, ny, nz, apix, False)

        expected_data = copy.deepcopy(test_data)
        expected_data[mask] = apix / expected_data[mask]
        expected_data[~mask] = 0
        print("EXP", expected_data)
        print("RET", returned_data.get_3dview())
        assert numpy.array_equal(expected_data, returned_data.get_3dview())
Exemplo n.º 8
0
def filterlocal(ui, vi, m, falloff, myid, main_node, number_of_proc):
	from mpi 	  	  import mpi_init, mpi_comm_size, mpi_comm_rank, MPI_COMM_WORLD
	from mpi 	  	  import mpi_reduce, mpi_bcast, mpi_barrier, mpi_gatherv, mpi_send, mpi_recv
	from mpi 	  	  import MPI_SUM, MPI_FLOAT, MPI_INT
	from sp_utilities import bcast_number_to_all, bcast_list_to_all, model_blank, bcast_EMData_to_all, reduce_EMData_to_root
	from sp_morphology import threshold_outside
	from sp_filter import filt_tanl
	from sp_fundamentals import fft, fftip

	if(myid == main_node):

		nx = vi.get_xsize()
		ny = vi.get_ysize()
		nz = vi.get_zsize()
		#  Round all resolution numbers to two digits
		for x in range(nx):
			for y in range(ny):
				for z in range(nz):
					ui.set_value_at_fast( x,y,z, round(ui.get_value_at(x,y,z), 2) )
		dis = [nx,ny,nz]
	else:
		falloff = 0.0
		radius  = 0
		dis = [0,0,0]
	falloff = bcast_number_to_all(falloff, main_node)
	dis = bcast_list_to_all(dis, myid, source_node = main_node)

	if(myid != main_node):
		nx = int(dis[0])
		ny = int(dis[1])
		nz = int(dis[2])

		vi = model_blank(nx,ny,nz)
		ui = model_blank(nx,ny,nz)

	bcast_EMData_to_all(vi, myid, main_node)
	bcast_EMData_to_all(ui, myid, main_node)

	fftip(vi)  #  volume to be filtered

	st = Util.infomask(ui, m, True)


	filteredvol = model_blank(nx,ny,nz)
	cutoff = max(st[2] - 0.01,0.0)
	while(cutoff < st[3] ):
		cutoff = round(cutoff + 0.01, 2)
		#if(myid == main_node):  print  cutoff,st
		pt = Util.infomask( threshold_outside(ui, cutoff - 0.00501, cutoff + 0.005), m, True)  # Ideally, one would want to check only slices in question...
		if(pt[0] != 0.0):
			#print cutoff,pt[0]
			vovo = fft( filt_tanl(vi, cutoff, falloff) )
			for z in range(myid, nz, number_of_proc):
				for x in range(nx):
					for y in range(ny):
						if(m.get_value_at(x,y,z) > 0.5):
							if(round(ui.get_value_at(x,y,z),2) == cutoff):
								filteredvol.set_value_at_fast(x,y,z,vovo.get_value_at(x,y,z))

	mpi_barrier(MPI_COMM_WORLD)
	reduce_EMData_to_root(filteredvol, myid, main_node, MPI_COMM_WORLD)
	return filteredvol
Exemplo n.º 9
0
def write_montage_file(stack, montage_file, N, gx, gy, bg, scale, number,
                       begin_zero):

    from sp_utilities import model_blank

    font = [
        "0011100010001010000011000001100000110000011000001100000101000100011100",
        "0001000001100001010001001000000100000010000001000000100000010001111111",
        "0111110100000110000010000001000001000001000011000010000001000001111111",
        "1111111000000100000100000100000111000000010000001000000110000010111110",
        "0000010000011000010100010010010001010000101111111000001000000100000010",
        "1111111100000010000001011110110000100000010000001000000110000010111110",
        "0011110010000010000001000000101111101100000110000011000001100000101111",
        "1111111000000100000010000010000010000100000100000010000010000010000000",
        "0011100010001010000010100010001110001000101000001100000101000010011100",
        "0111110100000011000001100000110000110111101000000100000010000010011110"
    ]

    if gy == -1: gy = gx

    data = EMData.read_images(stack)
    if scale:
        for im in data:
            st = Util.infomask(im, None, True)
            im -= st[0]
            im /= st[1]

    nx = data[0].get_xsize()
    ny = data[0].get_ysize()

    K = len(data)
    M = (K - 1) / N + 1

    NX = (nx + gx) * N
    NY = (ny + gy) * M

    maxn = -1.e-20
    minn = 1.e+20
    avgn = 0
    for im in data:
        st = Util.infomask(im, None, True)
        avgn += st[0]
        if st[3] > maxn: maxn = st[3]
        if st[2] < minn: minn = st[2]
    avgn /= K

    if bg == 0:
        bk = minn
    elif bg == 1:
        bk = maxn
    elif bg == 2:
        bk = 0
    else:
        bk = avgn

    montage = model_blank(NX, NY, 1, bk)

    for i in range(K):
        col = i % N
        row = M - 1 - i / N
        for s in range(nx):
            for t in range(ny):
                v = data[i].get_value_at(s, t)
                montage.set_value_at(col * (nx + gx) + s,
                                     row * (ny + gy) + t, v)
        if number:
            for s in range(10):
                for t in range(7):
                    if font[i % 10][s * 7 + t] == '1':
                        montage.set_value_at(col * (nx + gx) + 2 + t,
                                             row * (ny + gy) + 2 + 10 - s,
                                             maxn)
    montage.write_image(montage_file)
Exemplo n.º 10
0
def align2d_direct3(input_images,
                    refim,
                    xrng=1,
                    yrng=1,
                    psimax=180,
                    psistep=1,
                    ou=-1,
                    CTF=None):

    nx = input_images[0].get_xsize()
    if ou < 0:
        ou = old_div(nx, 2) - 1
    mask = sp_utilities.model_circle(ou, nx, nx)
    nk = int(old_div(psimax, psistep))
    nm = 2 * nk + 1
    nc = nk + 1
    refs = [None] * nm * 2
    for i in range(nm):
        temp = sp_fundamentals.rot_shift2D(refim, (i - nc) * psistep) * mask
        refs[2 * i] = [
            sp_fundamentals.fft(temp),
            sp_fundamentals.fft(sp_fundamentals.mirror(temp)),
        ]
        temp = sp_fundamentals.rot_shift2D(refim,
                                           (i - nc) * psistep + 180.0) * mask
        refs[2 * i + 1] = [
            sp_fundamentals.fft(temp),
            sp_fundamentals.fft(sp_fundamentals.mirror(temp)),
        ]
    del temp

    results = []
    mir = 0
    for image in input_images:
        if CTF:
            ims = sp_filter.filt_ctf(sp_fundamentals.fft(image),
                                     image.get_attr("ctf"))
        else:
            ims = sp_fundamentals.fft(image)
        ama = -1.0e23
        bang = 0.0
        bsx = 0.0
        bsy = 0.0
        for i in range(nm * 2):
            for mirror_flag in [0, 1]:
                c = sp_fundamentals.ccf(ims, refs[i][mirror_flag])
                w = EMAN2_cppwrap.Util.window(c, 2 * xrng + 1, 2 * yrng + 1)
                pp = sp_utilities.peak_search(w)[0]
                px = int(pp[4])
                py = int(pp[5])
                if pp[0] == 1.0 and px == 0 and py == 0:
                    pass  # XSH, YSH, PEAKV = 0.,0.,0.
                else:
                    ww = sp_utilities.model_blank(3, 3)
                    ux = int(pp[1])
                    uy = int(pp[2])
                    for k in range(3):
                        for l in range(3):
                            ww[k, l] = w[k + ux - 1, l + uy - 1]
                    XSH, YSH, PEAKV = parabl(ww)
                    # print i,pp[-1],XSH, YSH,px+XSH, py+YSH, PEAKV
                    if PEAKV > ama:
                        ama = PEAKV
                        bsx = px + round(XSH, 2)
                        bsy = py + round(YSH, 2)
                        bang = i
                        mir = mirror_flag
        # returned parameters have to be inverted
        bang = (old_div(bang, 2) - nc) * psistep + 180.0 * (bang % 2)
        bang, bsx, bsy, _ = sp_utilities.inverse_transform2(
            bang, (1 - 2 * mir) * bsx, bsy, mir)
        results.append([bang, bsx, bsy, mir, ama])
    return results
Exemplo n.º 11
0
def main():
    arglist = []
    for arg in sys.argv:
        arglist.append(arg)
    progname = optparse.os.path.basename(arglist[0])
    usage = progname + """ inputvolume  locresvolume maskfile outputfile   --radius --falloff  --MPI

	    Locally filer a volume based on local resolution volume (sxlocres.py) within area outlined by the maskfile
	"""
    parser = optparse.OptionParser(usage, version=sp_global_def.SPARXVERSION)

    parser.add_option(
        "--radius",
        type="int",
        default=-1,
        help=
        "if there is no maskfile, sphere with r=radius will be used, by default the radius is nx/2-1"
    )
    parser.add_option("--falloff",
                      type="float",
                      default=0.1,
                      help="falloff of tanl filter (default 0.1)")
    parser.add_option("--MPI",
                      action="store_true",
                      default=False,
                      help="use MPI version")

    (options, args) = parser.parse_args(arglist[1:])

    if len(args) < 3 or len(args) > 4:
        sp_global_def.sxprint("See usage " + usage)
        sp_global_def.ERROR(
            "Wrong number of parameters. Please see usage information above.")
        return

    if sp_global_def.CACHE_DISABLE:
        pass  #IMPORTIMPORTIMPORT from sp_utilities import disable_bdb_cache
        sp_utilities.disable_bdb_cache()

    if options.MPI:
        number_of_proc = mpi.mpi_comm_size(mpi.MPI_COMM_WORLD)
        myid = mpi.mpi_comm_rank(mpi.MPI_COMM_WORLD)
        main_node = 0

        if (myid == main_node):
            #print sys.argv
            vi = sp_utilities.get_im(sys.argv[1])
            ui = sp_utilities.get_im(sys.argv[2])
            #print   Util.infomask(ui, None, True)
            radius = options.radius
            nx = vi.get_xsize()
            ny = vi.get_ysize()
            nz = vi.get_zsize()
            dis = [nx, ny, nz]
        else:
            falloff = 0.0
            radius = 0
            dis = [0, 0, 0]
            vi = None
            ui = None
        dis = sp_utilities.bcast_list_to_all(dis, myid, source_node=main_node)

        if (myid != main_node):
            nx = int(dis[0])
            ny = int(dis[1])
            nz = int(dis[2])
        radius = sp_utilities.bcast_number_to_all(radius, main_node)
        if len(args) == 3:
            if (radius == -1):
                radius = min(nx, ny, nz) // 2 - 1
            m = sp_utilities.model_circle(radius, nx, ny, nz)
            outvol = args[2]

        elif len(args) == 4:
            if (myid == main_node):
                m = sp_morphology.binarize(sp_utilities.get_im(args[2]), 0.5)
            else:
                m = sp_utilities.model_blank(nx, ny, nz)
            outvol = args[3]
            sp_utilities.bcast_EMData_to_all(m, myid, main_node)

        pass  #IMPORTIMPORTIMPORT from sp_filter import filterlocal
        filteredvol = sp_filter.filterlocal(ui, vi, m, options.falloff, myid,
                                            main_node, number_of_proc)

        if (myid == 0):
            filteredvol.write_image(outvol)

    else:
        vi = sp_utilities.get_im(args[0])
        ui = sp_utilities.get_im(
            args[1]
        )  # resolution volume, values are assumed to be from 0 to 0.5

        nn = vi.get_xsize()

        falloff = options.falloff

        if len(args) == 3:
            radius = options.radius
            if (radius == -1):
                radius = nn // 2 - 1
            m = sp_utilities.model_circle(radius, nn, nn, nn)
            outvol = args[2]

        elif len(args) == 4:
            m = sp_morphology.binarize(sp_utilities.get_im(args[2]), 0.5)
            outvol = args[3]

        sp_fundamentals.fftip(vi)  # this is the volume to be filtered

        #  Round all resolution numbers to two digits
        for x in range(nn):
            for y in range(nn):
                for z in range(nn):
                    ui.set_value_at_fast(x, y, z,
                                         round(ui.get_value_at(x, y, z), 2))
        st = EMAN2_cppwrap.Util.infomask(ui, m, True)

        filteredvol = sp_utilities.model_blank(nn, nn, nn)
        cutoff = max(st[2] - 0.01, 0.0)
        while (cutoff < st[3]):
            cutoff = round(cutoff + 0.01, 2)
            pt = EMAN2_cppwrap.Util.infomask(
                sp_morphology.threshold_outside(ui, cutoff - 0.00501,
                                                cutoff + 0.005), m, True)
            if (pt[0] != 0.0):
                vovo = sp_fundamentals.fft(
                    sp_filter.filt_tanl(vi, cutoff, falloff))
                for x in range(nn):
                    for y in range(nn):
                        for z in range(nn):
                            if (m.get_value_at(x, y, z) > 0.5):
                                if (round(ui.get_value_at(x, y, z),
                                          2) == cutoff):
                                    filteredvol.set_value_at_fast(
                                        x, y, z, vovo.get_value_at(x, y, z))

        sp_global_def.write_command(optparse.os.path.dirname(outvol))
        filteredvol.write_image(outvol)
Exemplo n.º 12
0
def main():
    """
	Main function.

	Arguments:
	None

	Returns:
	None
	"""

    command_args = parse_command_line()

    # Import volume
    sp_global_def.sxprint("Import volume.")
    input_vol = sp_utilities.get_im(command_args.input_volume)

    # Sanity checks
    sanity_checks(command_args, input_vol)

    try:
        os.makedirs(command_args.output_dir)
    except OSError:
        sp_global_def.sxprint(
            "Output directory already exists. No need to create it.")
    else:
        sp_global_def.sxprint("Created output directory.")
    sp_global_def.write_command(command_args.output_dir)
    output_prefix = os.path.join(command_args.output_dir, command_args.prefix)

    # Filter volume if specified
    if command_args.low_pass_filter_resolution is not None:
        sp_global_def.sxprint("Filter volume to {0}A.".format(
            command_args.low_pass_filter_resolution))
        input_vol = sp_filter.filt_tanl(
            input_vol,
            old_div(command_args.pixel_size,
                    command_args.low_pass_filter_resolution),
            command_args.low_pass_filter_falloff,
        )
        input_vol.write_image(output_prefix + "_filtered_volume.hdf")
    else:
        sp_global_def.sxprint("Skip filter volume.")

    # Create a mask based on the filtered volume
    sp_global_def.sxprint("Create mask")
    density_threshold = -9999.0
    nsigma = 1.0
    if command_args.mol_mass:
        density_threshold = input_vol.find_3d_threshold(
            command_args.mol_mass, command_args.pixel_size)
        sp_global_def.sxprint(
            "Mask molecular mass translated into binary threshold: ",
            density_threshold)
    elif command_args.threshold:
        density_threshold = command_args.threshold
    elif command_args.nsigma:
        nsigma = command_args.nsigma
    else:
        assert False

    if command_args.edge_type == "cosine":
        mode = "C"
    elif command_args.edge_type == "gaussian":
        mode = "G"
    else:
        assert False

    mask_first = sp_morphology.adaptive_mask_scipy(
        input_vol,
        nsigma=nsigma,
        threshold=density_threshold,
        ndilation=command_args.ndilation,
        nerosion=command_args.nerosion,
        edge_width=command_args.edge_width,
        allow_disconnected=command_args.allow_disconnected,
        mode=mode,
        do_approx=command_args.do_old,
        do_fill=command_args.fill_mask,
        do_print=True,
    )

    # Create a second mask based on the filtered volume
    s_mask = None
    s_density_threshold = 1
    s_nsigma = 1.0
    if command_args.second_mask is not None:
        sp_global_def.sxprint("Prepare second mask")
        s_mask = sp_utilities.get_im(command_args.second_mask)
        s_density_threshold = -9999.0
        s_nsigma = 1.0
        if command_args.s_mol_mass:
            s_density_threshold = input_vol.find_3d_threshold(
                command_args.s_mol_mass, command_args.s_pixel_size)
            sp_global_def.sxprint(
                "Second mask molecular mass translated into binary threshold: ",
                s_density_threshold,
            )
        elif command_args.s_threshold:
            s_density_threshold = command_args.s_threshold
        elif command_args.s_nsigma:
            s_nsigma = command_args.s_nsigma
        else:
            assert False
    elif command_args.second_mask_shape is not None:
        sp_global_def.sxprint("Prepare second mask")
        nx = mask_first.get_xsize()
        ny = mask_first.get_ysize()
        nz = mask_first.get_zsize()
        if command_args.second_mask_shape == "cube":
            s_nx = command_args.s_nx
            s_ny = command_args.s_ny
            s_nz = command_args.s_nz
            s_mask = sp_utilities.model_blank(s_nx, s_ny, s_nz, 1)
        elif command_args.second_mask_shape == "cylinder":
            s_radius = command_args.s_radius
            s_nx = command_args.s_nx
            s_ny = command_args.s_ny
            s_nz = command_args.s_nz
            try:
                s_mask = sp_utilities.model_cylinder(s_radius, s_nx, s_ny,
                                                     s_nz)
            except RuntimeError as e:
                sp_global_def.sxprint(
                    "An error occured! Please check the error log")
                raise
        elif command_args.second_mask_shape == "sphere":
            s_radius = command_args.s_radius
            s_nx = command_args.s_nx
            s_ny = command_args.s_ny
            s_nz = command_args.s_nz
            try:
                s_mask = sp_utilities.model_circle(s_radius, s_nx, s_ny, s_nz)
            except RuntimeError as e:
                sp_global_def.sxprint(
                    "An error occured! Please check the error log")
                raise
        else:
            assert False
        s_mask = sp_utilities.pad(s_mask, nx, ny, nz, 0)

    if s_mask is not None:
        sp_global_def.sxprint("Create second mask")

        if command_args.s_edge_type == "cosine":
            mode = "C"
        elif command_args.s_edge_type == "gaussian":
            mode = "G"
        else:
            assert False

        s_mask = sp_morphology.adaptive_mask_scipy(
            s_mask,
            nsigma=s_nsigma,
            threshold=s_density_threshold,
            ndilation=command_args.s_ndilation,
            nerosion=command_args.s_nerosion,
            edge_width=command_args.s_edge_width,
            allow_disconnected=command_args.s_allow_disconnected,
            mode=mode,
            do_approx=command_args.s_do_old,
            do_fill=command_args.s_fill_mask,
            do_print=True,
        )
        if command_args.s_invert:
            s_mask = 1 - s_mask
        sp_global_def.sxprint("Write outputs.")
        mask_first.write_image(output_prefix + "_mask_first.hdf")
        s_mask.write_image(output_prefix + "_mask_second.hdf")
        masked_combined = mask_first * s_mask
        masked_combined.write_image(output_prefix + "_mask.hdf")
    else:
        sp_global_def.sxprint("Write outputs.")
        mask_first.write_image(output_prefix + "_mask.hdf")
Exemplo n.º 13
0
def recons3d_4nn_ctf_MPI(
    myid,
    prjlist,
    snr=1.0,
    sign=1,
    symmetry="c1",
    finfo=None,
    npad=2,
    xysize=-1,
    zsize=-1,
    mpi_comm=None,
    smearstep=0.0,
):
    """
		recons3d_4nn_ctf - calculate CTF-corrected 3-D reconstruction from a set of projections using three Eulerian angles, two shifts, and CTF settings for each projeciton image
		Input
			stack: name of the stack file containing projection data, projections have to be squares
			list_proj: list of projections to be included in the reconstruction or image iterator
			snr: Signal-to-Noise Ratio of the data
			sign: sign of the CTF
			symmetry: point-group symmetry to be enforced, each projection will enter the reconstruction in all symmetry-related directions.
	"""

    if mpi_comm == None:
        mpi_comm = mpi.MPI_COMM_WORLD

    if type(prjlist) == list:
        prjlist = sp_utilities.iterImagesList(prjlist)
    if not prjlist.goToNext():
        sp_global_def.ERROR("empty input list", "recons3d_4nn_ctf_MPI", 1)
    imgsize = prjlist.image().get_xsize()
    if prjlist.image().get_ysize() != imgsize:
        imgsize = max(imgsize, prjlist.image().get_ysize())
        dopad = True
    else:
        dopad = False
    prjlist.goToPrev()

    fftvol = EMAN2_cppwrap.EMData()

    if smearstep > 0.0:
        # if myid == 0:  print "  Setting smear in prepare_recons_ctf"
        ns = 1
        smear = []
        for j in range(-ns, ns + 1):
            if j != 0:
                for i in range(-ns, ns + 1):
                    for k in range(-ns, ns + 1):
                        smear += [
                            i * smearstep, j * smearstep, k * smearstep, 1.0
                        ]
        # Deal with theta = 0.0 cases
        prj = []
        for i in range(-ns, ns + 1):
            for k in range(-ns, ns + 1):
                prj.append(i + k)
        for i in range(-2 * ns, 2 * ns + 1, 1):
            smear += [i * smearstep, 0.0, 0.0, float(prj.count(i))]
        # if myid == 0:  print "  Smear  ",smear
        fftvol.set_attr("smear", smear)

    weight = EMAN2_cppwrap.EMData()
    if xysize == -1 and zsize == -1:
        params = {
            "size": imgsize,
            "npad": npad,
            "snr": snr,
            "sign": sign,
            "symmetry": symmetry,
            "fftvol": fftvol,
            "weight": weight,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4_ctf", params)
    else:
        if xysize != -1 and zsize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = old_div(float(zsize), imgsize)
        elif xysize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = 1.0
        else:
            rx = 1.0
            ry = 1.0
            rz = old_div(float(zsize), imgsize)
        #  There is an error here with sizeprojection  PAP 10/22/2014
        params = {
            "size": sizeprojection,
            "npad": npad,
            "snr": snr,
            "sign": sign,
            "symmetry": symmetry,
            "fftvol": fftvol,
            "weight": weight,
            "xratio": rx,
            "yratio": ry,
            "zratio": rz,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4_ctf_rect", params)
    r.setup()

    # if not (finfo is None):
    nimg = 0
    while prjlist.goToNext():
        prj = prjlist.image()
        if dopad:
            prj = sp_utilities.pad(prj, imgsize, imgsize, 1, "circumference")
        # if params:
        insert_slices(r, prj)
        if not (finfo is None):
            nimg += 1
            finfo.write(" %4d inserted\n" % (nimg))
            finfo.flush()
    del sp_utilities.pad
    if not (finfo is None):
        finfo.write("begin reduce\n")
        finfo.flush()

    sp_utilities.reduce_EMData_to_root(fftvol, myid, comm=mpi_comm)
    sp_utilities.reduce_EMData_to_root(weight, myid, comm=mpi_comm)

    if not (finfo is None):
        finfo.write("after reduce\n")
        finfo.flush()

    if myid == 0:
        dummy = r.finish(True)
    else:
        if xysize == -1 and zsize == -1:
            fftvol = sp_utilities.model_blank(imgsize, imgsize, imgsize)
        else:
            if zsize == -1:
                fftvol = sp_utilities.model_blank(xysize, xysize, imgsize)
            elif xysize == -1:
                fftvol = sp_utilities.model_blank(imgsize, imgsize, zsize)
            else:
                fftvol = sp_utilities.model_blank(xysize, xysize, zsize)
    return fftvol
Exemplo n.º 14
0
def recons3d_trl_struct_MPI(
    myid,
    main_node,
    prjlist,
    paramstructure,
    refang,
    rshifts_shrank,
    delta,
    upweighted=True,
    mpi_comm=None,
    CTF=True,
    target_size=-1,
    avgnorm=1.0,
    norm_per_particle=None,
):
    """
		recons3d_4nn_ctf - calculate CTF-corrected 3-D reconstruction from a set of projections using three Eulerian angles, two shifts, and CTF settings for each projeciton image
		Input
			list_of_prjlist: list of lists of projections to be included in the reconstruction
	"""

    if mpi_comm == None:
        mpi_comm = mpi.MPI_COMM_WORLD

    refvol = sp_utilities.model_blank(target_size)
    refvol.set_attr("fudge", 1.0)

    if CTF:
        do_ctf = 1
    else:
        do_ctf = 0

    fftvol = EMAN2_cppwrap.EMData()
    weight = EMAN2_cppwrap.EMData()

    params = {
        "size": target_size,
        "npad": 2,
        "snr": 1.0,
        "sign": 1,
        "symmetry": "c1",
        "refvol": refvol,
        "fftvol": fftvol,
        "weight": weight,
        "do_ctf": do_ctf,
    }
    r = EMAN2_cppwrap.Reconstructors.get("nn4_ctfw", params)
    r.setup()

    if prjlist:
        if norm_per_particle == None:
            norm_per_particle = len(prjlist) * [1.0]

        nnx = prjlist[0].get_xsize()
        nny = prjlist[0].get_ysize()
        nshifts = len(rshifts_shrank)
        for im in range(len(prjlist)):
            #  parse projection structure, generate three lists:
            #  [ipsi+iang], [ishift], [probability]
            #  Number of orientations for a given image
            numbor = len(paramstructure[im][2])
            ipsiandiang = [
                old_div(paramstructure[im][2][i][0], 1000)
                for i in range(numbor)
            ]
            allshifts = [
                paramstructure[im][2][i][0] % 1000 for i in range(numbor)
            ]
            probs = [paramstructure[im][2][i][1] for i in range(numbor)]
            #  Find unique projection directions
            tdir = list(set(ipsiandiang))
            bckgn = prjlist[im].get_attr("bckgnoise")
            ct = prjlist[im].get_attr("ctf")
            #  For each unique projection direction:
            data = [None] * nshifts
            for ii in range(len(tdir)):
                #  Find the number of times given projection direction appears on the list, it is the number of different shifts associated with it.
                lshifts = sp_utilities.findall(tdir[ii], ipsiandiang)
                toprab = 0.0
                for ki in range(len(lshifts)):
                    toprab += probs[lshifts[ki]]
                recdata = EMAN2_cppwrap.EMData(nny, nny, 1, False)
                recdata.set_attr("is_complex", 0)
                for ki in range(len(lshifts)):
                    lpt = allshifts[lshifts[ki]]
                    if data[lpt] == None:
                        data[lpt] = sp_fundamentals.fshift(
                            prjlist[im], rshifts_shrank[lpt][0],
                            rshifts_shrank[lpt][1])
                        data[lpt].set_attr("is_complex", 0)
                    EMAN2_cppwrap.Util.add_img(
                        recdata,
                        EMAN2_cppwrap.Util.mult_scalar(
                            data[lpt], old_div(probs[lshifts[ki]], toprab)),
                    )
                recdata.set_attr_dict({
                    "padffted": 1,
                    "is_fftpad": 1,
                    "is_fftodd": 0,
                    "is_complex_ri": 1,
                    "is_complex": 1,
                })
                if not upweighted:
                    recdata = sp_filter.filt_table(recdata, bckgn)
                recdata.set_attr_dict({"bckgnoise": bckgn, "ctf": ct})
                ipsi = tdir[ii] % 100000
                iang = old_div(tdir[ii], 100000)
                r.insert_slice(
                    recdata,
                    EMAN2_cppwrap.Transform({
                        "type":
                        "spider",
                        "phi":
                        refang[iang][0],
                        "theta":
                        refang[iang][1],
                        "psi":
                        refang[iang][2] + ipsi * delta,
                    }),
                    old_div(toprab * avgnorm, norm_per_particle[im]),
                )
        #  clean stuff
        del bckgn, recdata, tdir, ipsiandiang, allshifts, probs

    sp_utilities.reduce_EMData_to_root(fftvol, myid, main_node, comm=mpi_comm)
    sp_utilities.reduce_EMData_to_root(weight, myid, main_node, comm=mpi_comm)

    if myid == main_node:
        dummy = r.finish(True)
    mpi.mpi_barrier(mpi_comm)

    if myid == main_node:
        return fftvol, weight, refvol
    else:
        return None, None, None
Exemplo n.º 15
0
def recons3d_4nnw_MPI(
    myid,
    prjlist,
    bckgdata,
    snr=1.0,
    sign=1,
    symmetry="c1",
    finfo=None,
    npad=2,
    xysize=-1,
    zsize=-1,
    mpi_comm=None,
    smearstep=0.0,
    fsc=None,
):
    """
		recons3d_4nn_ctf - calculate CTF-corrected 3-D reconstruction from a set of projections using three Eulerian angles, two shifts, and CTF settings for each projeciton image
		Input
			stack: name of the stack file containing projection data, projections have to be squares
			prjlist: list of projections to be included in the reconstruction or image iterator
			bckgdata = [get_im("tsd.hdf"),read_text_file("data_stamp.txt")]
			snr: Signal-to-Noise Ratio of the data
			sign: sign of the CTF
			symmetry: point-group symmetry to be enforced, each projection will enter the reconstruction in all symmetry-related directions.
	"""
    pass  # IMPORTIMPORTIMPORT from sp_utilities  import reduce_EMData_to_root, pad
    pass  # IMPORTIMPORTIMPORT from EMAN2      import Reconstructors
    pass  # IMPORTIMPORTIMPORT from sp_utilities  import iterImagesList, set_params_proj, model_blank
    pass  # IMPORTIMPORTIMPORT from mpi        import MPI_COMM_WORLD
    pass  # IMPORTIMPORTIMPORT import types

    if mpi_comm == None:
        mpi_comm = mpi.MPI_COMM_WORLD

    if type(prjlist) == list:
        prjlist = sp_utilities.iterImagesList(prjlist)
    if not prjlist.goToNext():
        sp_global_def.ERROR("empty input list", "recons3d_4nnw_MPI", 1)
    imgsize = prjlist.image().get_xsize()
    if prjlist.image().get_ysize() != imgsize:
        imgsize = max(imgsize, prjlist.image().get_ysize())
        dopad = True
    else:
        dopad = False
    prjlist.goToPrev()

    #  Do the FSC shtick.
    bnx = old_div(imgsize * npad, 2) + 1
    if fsc:
        pass  # IMPORTIMPORTIMPORT from math import sqrt
        pass  # IMPORTIMPORTIMPORT from sp_utilities import reshape_1d
        t = [0.0] * len(fsc)
        for i in range(len(fsc)):
            t[i] = min(max(fsc[i], 0.0), 0.999)
        t = sp_utilities.reshape_1d(t, len(t), npad * len(t))
        refvol = sp_utilities.model_blank(bnx, 1, 1, 0.0)
        for i in range(len(fsc)):
            refvol.set_value_at(i, t[i])
    else:
        refvol = sp_utilities.model_blank(bnx, 1, 1, 1.0)
    refvol.set_attr("fudge", 1.0)

    fftvol = EMAN2_cppwrap.EMData()
    weight = EMAN2_cppwrap.EMData()

    if smearstep > 0.0:
        # if myid == 0:  print "  Setting smear in prepare_recons_ctf"
        ns = 1
        smear = []
        for j in range(-ns, ns + 1):
            if j != 0:
                for i in range(-ns, ns + 1):
                    for k in range(-ns, ns + 1):
                        smear += [
                            i * smearstep, j * smearstep, k * smearstep, 1.0
                        ]
        # Deal with theta = 0.0 cases
        prj = []
        for i in range(-ns, ns + 1):
            for k in range(-ns, ns + 1):
                prj.append(i + k)
        for i in range(-2 * ns, 2 * ns + 1, 1):
            smear += [i * smearstep, 0.0, 0.0, float(prj.count(i))]
        # if myid == 0:  print "  Smear  ",smear
        fftvol.set_attr("smear", smear)

    if xysize == -1 and zsize == -1:
        params = {
            "size": imgsize,
            "npad": npad,
            "snr": snr,
            "sign": sign,
            "symmetry": symmetry,
            "refvol": refvol,
            "fftvol": fftvol,
            "weight": weight,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4_ctfw", params)
    else:
        if xysize != -1 and zsize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = old_div(float(zsize), imgsize)
        elif xysize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = 1.0
        else:
            rx = 1.0
            ry = 1.0
            rz = old_div(float(zsize), imgsize)
        #  There is an error here with sizeprojection  PAP 10/22/2014
        params = {
            "size": sizeprojection,
            "npad": npad,
            "snr": snr,
            "sign": sign,
            "symmetry": symmetry,
            "fftvol": fftvol,
            "weight": weight,
            "xratio": rx,
            "yratio": ry,
            "zratio": rz,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4_ctf_rect", params)
    r.setup()

    # from utilities import model_blank, get_im, read_text_file
    # bckgdata = [get_im("tsd.hdf"),read_text_file("data_stamp.txt")]

    nnx = bckgdata[0].get_xsize()
    nny = bckgdata[0].get_ysize()
    bckgnoise = []
    for i in range(nny):
        prj = sp_utilities.model_blank(nnx)
        for k in range(nnx):
            prj[k] = bckgdata[0].get_value_at(k, i)
        bckgnoise.append(prj)

    datastamp = bckgdata[1]
    if not (finfo is None):
        nimg = 0
    while prjlist.goToNext():
        prj = prjlist.image()
        try:
            stmp = old_div(nnx, 0)
            stmp = prj.get_attr("ptcl_source_image")
        except:
            try:
                stmp = prj.get_attr("ctf")
                stmp = round(stmp.defocus, 4)
            except:
                sp_global_def.ERROR(
                    "Either ptcl_source_image or ctf has to be present in the header.",
                    "recons3d_4nnw_MPI",
                    1,
                    myid,
                )
        try:
            indx = datastamp.index(stmp)
        except:
            sp_global_def.ERROR("Problem with indexing ptcl_source_image.",
                                "recons3d_4nnw_MPI", 1, myid)

        if dopad:
            prj = sp_utilities.pad(prj, imgsize, imgsize, 1, "circumference")

        prj.set_attr("bckgnoise", bckgnoise[indx])
        insert_slices(r, prj)
        if not (finfo is None):
            nimg += 1
            finfo.write(" %4d inserted\n" % (nimg))
            finfo.flush()
    del sp_utilities.pad
    if not (finfo is None):
        finfo.write("begin reduce\n")
        finfo.flush()

    sp_utilities.reduce_EMData_to_root(fftvol, myid, comm=mpi_comm)
    sp_utilities.reduce_EMData_to_root(weight, myid, comm=mpi_comm)

    if not (finfo is None):
        finfo.write("after reduce\n")
        finfo.flush()

    if myid == 0:
        dummy = r.finish(True)
    else:
        pass  # IMPORTIMPORTIMPORT from sp_utilities import model_blank
        if xysize == -1 and zsize == -1:
            fftvol = sp_utilities.model_blank(imgsize, imgsize, imgsize)
        else:
            if zsize == -1:
                fftvol = sp_utilities.model_blank(xysize, xysize, imgsize)
            elif xysize == -1:
                fftvol = sp_utilities.model_blank(imgsize, imgsize, zsize)
            else:
                fftvol = sp_utilities.model_blank(xysize, xysize, zsize)
    return fftvol
Exemplo n.º 16
0
def recons3d_4nn_MPI(
    myid,
    prjlist,
    symmetry="c1",
    finfo=None,
    snr=1.0,
    npad=2,
    xysize=-1,
    zsize=-1,
    mpi_comm=None,
):
    if mpi_comm == None:
        mpi_comm = mpi.MPI_COMM_WORLD

    if type(prjlist) == list:
        prjlist = sp_utilities.iterImagesList(prjlist)

    if not prjlist.goToNext():
        sp_global_def.ERROR("empty input list", "recons3d_4nn_MPI", 1)

    imgsize = prjlist.image().get_xsize()
    if prjlist.image().get_ysize() != imgsize:
        imgsize = max(imgsize, prjlist.image().get_ysize())
        dopad = True
    else:
        dopad = False
    prjlist.goToPrev()

    fftvol = EMAN2_cppwrap.EMData()
    weight = EMAN2_cppwrap.EMData()
    if xysize == -1 and zsize == -1:
        params = {
            "size": imgsize,
            "npad": npad,
            "symmetry": symmetry,
            "fftvol": fftvol,
            "weight": weight,
            "snr": snr,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4", params)
    else:
        if xysize != -1 and zsize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = old_div(float(zsize), imgsize)
        elif xysize != -1:
            rx = old_div(float(xysize), imgsize)
            ry = old_div(float(xysize), imgsize)
            rz = 1.0
        else:
            rx = 1.0
            ry = 1.0
            rz = old_div(float(zsize), imgsize)
        params = {
            "sizeprojection": imgsize,
            "npad": npad,
            "symmetry": symmetry,
            "fftvol": fftvol,
            "weight": weight,
            "xratio": rx,
            "yratio": ry,
            "zratio": rz,
        }
        r = EMAN2_cppwrap.Reconstructors.get("nn4_rect", params)
    r.setup()

    if not (finfo is None):
        nimg = 0
    while prjlist.goToNext():
        prj = prjlist.image()
        if dopad:
            prj = sp_utilities.pad(prj, imgsize, imgsize, 1, "circumference")
        insert_slices(r, prj)
        if not (finfo is None):
            nimg += 1
            finfo.write("Image %4d inserted.\n" % (nimg))
            finfo.flush()

    if not (finfo is None):
        finfo.write("Begin reducing ...\n")
        finfo.flush()

    sp_utilities.reduce_EMData_to_root(fftvol, myid, comm=mpi_comm)
    sp_utilities.reduce_EMData_to_root(weight, myid, comm=mpi_comm)

    if myid == 0:
        dummy = r.finish(True)
    else:
        if xysize == -1 and zsize == -1:
            fftvol = sp_utilities.model_blank(imgsize, imgsize, imgsize)
        else:
            if zsize == -1:
                fftvol = sp_utilities.model_blank(xysize, xysize, imgsize)
            elif xysize == -1:
                fftvol = sp_utilities.model_blank(imgsize, imgsize, zsize)
            else:
                fftvol = sp_utilities.model_blank(xysize, xysize, zsize)
    return fftvol
Exemplo n.º 17
0
def multalign2d_scf(image, refrings, frotim, numr, xrng=-1, yrng=-1, ou=-1):

    nx = image.get_xsize()
    ny = image.get_xsize()
    if ou < 0:
        ou = min(old_div(nx, 2) - 1, old_div(ny, 2) - 1)
    if yrng < 0:
        yrng = xrng
    if ou < 2:
        sp_global_def.ERROR("Radius of the object (ou) has to be given",
                            "align2d_scf", 1)
    sci = sp_fundamentals.scf(image)
    first_ring = 1
    # center in SPIDER convention
    cnx = old_div(nx, 2) + 1
    cny = old_div(ny, 2) + 1

    cimage = EMAN2_cppwrap.Util.Polar2Dm(sci, cnx, cny, numr, "H")
    EMAN2_cppwrap.Util.Frngs(cimage, numr)
    mimage = EMAN2_cppwrap.Util.Polar2Dm(sp_fundamentals.mirror(sci), cnx, cny,
                                         numr, "H")
    EMAN2_cppwrap.Util.Frngs(mimage, numr)

    nrx = min(2 * (xrng + 1) + 1, ((old_div((nx - 2), 2)) * 2 + 1))
    nry = min(2 * (yrng + 1) + 1, ((old_div((ny - 2), 2)) * 2 + 1))

    totpeak = -1.0e23

    for iki in range(len(refrings)):
        # print  "TEMPLATE  ",iki
        #  Find angle
        retvals = EMAN2_cppwrap.Util.Crosrng_e(refrings[iki], cimage, numr, 0,
                                               0.0)
        alpha1 = ang_n(retvals["tot"], "H", numr[-1])
        peak1 = retvals["qn"]
        retvals = EMAN2_cppwrap.Util.Crosrng_e(refrings[iki], mimage, numr, 0,
                                               0.0)
        alpha2 = ang_n(retvals["tot"], "H", numr[-1])
        peak2 = retvals["qn"]
        # print  alpha1, peak1
        # print  alpha2, peak2

        if peak1 > peak2:
            mirr = 0
            alpha = alpha1
        else:
            mirr = 1
            alpha = -alpha2

        ccf1 = EMAN2_cppwrap.Util.window(
            sp_fundamentals.ccf(
                sp_fundamentals.rot_shift2D(image, alpha, 0.0, 0.0, mirr),
                frotim[iki]),
            nrx,
            nry,
        )
        p1 = sp_utilities.peak_search(ccf1)

        ccf2 = EMAN2_cppwrap.Util.window(
            sp_fundamentals.ccf(
                sp_fundamentals.rot_shift2D(image, alpha + 180.0, 0.0, 0.0,
                                            mirr),
                frotim[iki],
            ),
            nrx,
            nry,
        )
        p2 = sp_utilities.peak_search(ccf2)
        # print p1
        # print p2

        peak_val1 = p1[0][0]
        peak_val2 = p2[0][0]

        if peak_val1 > peak_val2:
            sxs = -p1[0][4]
            sys = -p1[0][5]
            cx = int(p1[0][1])
            cy = int(p1[0][2])
            peak = peak_val1
        else:
            alpha += 180.0
            sxs = -p2[0][4]
            sys = -p2[0][5]
            peak = peak_val2
            cx = int(p2[0][1])
            cy = int(p2[0][2])
            ccf1 = ccf2
        # print cx,cy
        z = sp_utilities.model_blank(3, 3)
        for i in range(3):
            for j in range(3):
                z[i, j] = ccf1[i + cx - 1, j + cy - 1]
        # print  ccf1[cx,cy],z[1,1]
        XSH, YSH, PEAKV = parabl(z)
        # print  PEAKV
        if PEAKV > totpeak:
            totpeak = PEAKV
            iref = iki
            if mirr == 1:
                sx = -sxs + XSH
            else:
                sx = sxs - XSH
            sy = sys - YSH
            talpha = alpha
            tmirr = mirr
            # print "BETTER",sx,sy,iref,talpha,tmirr,totpeak
            # return alpha, sx, sys-YSH, mirr, PEAKV
    return sx, sy, iref, talpha, tmirr, totpeak
Exemplo n.º 18
0
def align2d_scf(image, refim, xrng=-1, yrng=-1, ou=-1):
    nx = image.get_xsize()
    ny = image.get_xsize()
    if ou < 0:
        ou = min(old_div(nx, 2) - 1, old_div(ny, 2) - 1)
    if yrng < 0:
        yrng = xrng
    if ou < 2:
        sp_global_def.ERROR("Radius of the object (ou) has to be given",
                            "align2d_scf", 1)
    sci = sp_fundamentals.scf(image)
    scr = sp_fundamentals.scf(refim)
    first_ring = 1

    # alpha1, sxs, sys, mirr, peak1 = align2d_no_mirror(scf(image), scr, last_ring=ou, mode="H")
    # alpha2, sxs, sys, mirr, peak2 = align2d_no_mirror(scf(mirror(image)), scr, last_ring=ou, mode="H")
    # alpha1, sxs, sys, mirr, peak1 = align2d_no_mirror(sci, scr, first_ring = 1, last_ring=ou, mode="H")
    # alpha2, sxs, sys, mirr, peak2 = align2d_no_mirror(mirror(sci), scr,  first_ring = 1, last_ring=ou, mode="H")

    # center in SPIDER convention
    cnx = old_div(nx, 2) + 1
    cny = old_div(ny, 2) + 1
    # precalculate rings
    numr = Numrinit(first_ring, ou, 1, "H")
    wr = ringwe(numr, "H")
    crefim = EMAN2_cppwrap.Util.Polar2Dm(scr, cnx, cny, numr, "H")
    EMAN2_cppwrap.Util.Frngs(crefim, numr)
    EMAN2_cppwrap.Util.Applyws(crefim, numr, wr)
    alpha1, sxs, sys, mirr, peak1 = ornq(sci, crefim, [0.0], [0.0], 1.0, "H",
                                         numr, cnx, cny)
    alpha2, sxs, sys, mirr, peak2 = ornq(sp_fundamentals.mirror(sci), crefim,
                                         [0.0], [0.0], 1.0, "H", numr, cnx,
                                         cny)

    if peak1 > peak2:
        mirr = 0
        alpha = alpha1
    else:
        mirr = 1
        alpha = -alpha2
    nrx = min(2 * (xrng + 1) + 1, ((old_div((nx - 2), 2)) * 2 + 1))
    nry = min(2 * (yrng + 1) + 1, ((old_div((ny - 2), 2)) * 2 + 1))
    frotim = sp_fundamentals.fft(refim)
    ccf1 = EMAN2_cppwrap.Util.window(
        sp_fundamentals.ccf(
            sp_fundamentals.rot_shift2D(image, alpha, 0.0, 0.0, mirr), frotim),
        nrx,
        nry,
    )
    p1 = sp_utilities.peak_search(ccf1)

    ccf2 = EMAN2_cppwrap.Util.window(
        sp_fundamentals.ccf(
            sp_fundamentals.rot_shift2D(image, alpha + 180.0, 0.0, 0.0, mirr),
            frotim),
        nrx,
        nry,
    )
    p2 = sp_utilities.peak_search(ccf2)
    # print p1
    # print p2

    peak_val1 = p1[0][0]
    peak_val2 = p2[0][0]

    if peak_val1 > peak_val2:
        sxs = -p1[0][4]
        sys = -p1[0][5]
        cx = int(p1[0][1])
        cy = int(p1[0][2])
        peak = peak_val1
    else:
        alpha += 180.0
        sxs = -p2[0][4]
        sys = -p2[0][5]
        peak = peak_val2
        cx = int(p2[0][1])
        cy = int(p2[0][2])
        ccf1 = ccf2
    # print cx,cy
    z = sp_utilities.model_blank(3, 3)
    for i in range(3):
        for j in range(3):
            z[i, j] = ccf1[i + cx - 1, j + cy - 1]
    # print  ccf1[cx,cy],z[1,1]
    XSH, YSH, PEAKV = parabl(z)
    # print sxs, sys, XSH, YSH, PEAKV, peak
    if mirr == 1:
        sx = -sxs + XSH
    else:
        sx = sxs - XSH
    return alpha, sx, sys - YSH, mirr, PEAKV
Exemplo n.º 19
0
def generate_helimic(refvol,
                     outdir,
                     pixel,
                     CTF=False,
                     Cs=2.0,
                     voltage=200.0,
                     ampcont=10.0,
                     nonoise=False,
                     rand_seed=14567):

    from sp_utilities import model_blank, model_gauss, model_gauss_noise, pad, get_im
    from random import random
    from sp_projection import prgs, prep_vol
    from sp_filter import filt_gaussl, filt_ctf
    from EMAN2 import EMAN2Ctf

    if os.path.exists(outdir):
        ERROR(
            "Output directory exists, please change the name and restart the program"
        )
        return

    os.mkdir(outdir)
    seed(rand_seed)
    Util.set_randnum_seed(rand_seed)
    angles = []
    for i in range(3):
        angles.append([0.0 + 60.0 * i, 90.0 - i * 5, 0.0, 0.0, 0.0])

    nangle = len(angles)

    volfts = get_im(refvol)
    nx = volfts.get_xsize()
    ny = volfts.get_ysize()
    nz = volfts.get_zsize()
    volfts, kbx, kby, kbz = prep_vol(volfts)
    iprj = 0
    width = 500
    xstart = 0
    ystart = 0

    for idef in range(3, 6):
        mic = model_blank(2048, 2048)
        #defocus = idef*0.2
        defocus = idef * 0.6  ##@ming
        if CTF:
            #ctf = EMAN2Ctf()
            #ctf.from_dict( {"defocus":defocus, "cs":Cs, "voltage":voltage, "apix":pixel, "ampcont":ampcont, "bfactor":0.0} )
            from sp_utilities import generate_ctf
            ctf = generate_ctf(
                [defocus, 2, 200, 1.84, 0.0, ampcont, defocus * 0.2, 80]
            )  ##@ming   the range of astigmatism amplitude is between 10 percent and 22 percent. 20 percent is a good choice.
        i = idef - 4
        for k in range(1):
            psi = 90 + 10 * i
            proj = prgs(
                volfts, kbz,
                [angles[idef - 3][0], angles[idef - 3][1], psi, 0.0, 0.0], kbx,
                kby)
            proj = Util.window(proj, 320, nz)
            mic += pad(proj, 2048, 2048, 1, 0.0, 750 * i, 20 * i, 0)

        if not nonoise: mic += model_gauss_noise(30.0, 2048, 2048)
        if CTF:
            #apply CTF
            mic = filt_ctf(mic, ctf)

        if not nonoise:
            mic += filt_gaussl(model_gauss_noise(17.5, 2048, 2048), 0.3)

        mic.write_image("%s/mic%1d.hdf" % (outdir, idef - 3), 0)
Exemplo n.º 20
0
def main():
    progname = os.path.basename(sys.argv[0])
    usage = progname + """ Input Output [options]
	
	Generate three micrographs, each micrograph contains one projection of a long filament.
	Input: Reference Volume, output directory 
	Output: Three micrographs stored in output directory		
				 
		sxhelical_demo.py tmp.hdf  mic --generate_micrograph --CTF --apix=1.84	
	
	Generate noisy cylinder ini.hdf with radius 35 pixels and box size 100 by 100 by 200
	
		sxhelical_demo.py ini.hdf --generate_noisycyl --boxsize="100,100,200" --rad=35
	
	Generate rectangular 2D mask mask2d.hdf with width 60 pixels and image size 200 by 200 pixels
	
		sxhelical_demo.py mask2d.hdf --generate_mask --masksize="200,200" --maskwidth=60
	
	Apply the centering parameters to bdb:adata, normalize using average and standard deviation outside the mask, and output the new images to bdb:data
		
		sxhelical_demo.py bdb:adata bdb:data mask2d.hdf --applyparams
	
	Generate run through example script for helicon
	
		sxhelical_demo.py --generate_script --filename=run --seg_ny=180 --ptcl_dist=15 --fract=0.35
	"""
    parser = OptionParser(usage, version=SPARXVERSION)

    # helicise the Atom coordinates

    # generate micrographs of helical filament
    parser.add_option(
        "--generate_micrograph",
        action="store_true",
        default=False,
        help=
        "Generate three micrographs where each micrograph contains one projection of a long filament. \n Input: Reference Volume, output directory \n Output: Three micrographs containing helical filament projections stored in output directory"
    )
    parser.add_option("--CTF",
                      action="store_true",
                      default=False,
                      help="Use CTF correction")
    parser.add_option("--apix",
                      type="float",
                      default=-1,
                      help="pixel size in Angstroms")
    parser.add_option(
        "--rand_seed",
        type="int",
        default=14567,
        help=
        "the seed used for generating random numbers (default 14567) for adding noise to the generated micrographs."
    )
    parser.add_option("--Cs",
                      type="float",
                      default=2.0,
                      help="Microscope Cs (spherical aberation)")
    parser.add_option("--voltage",
                      type="float",
                      default=200.0,
                      help="Microscope voltage in KV")
    parser.add_option("--ac",
                      type="float",
                      default=10.0,
                      help="Amplitude contrast (percentage, default=10)")
    parser.add_option("--nonoise",
                      action="store_true",
                      default=False,
                      help="Do not add noise to the micrograph.")

    # generate initial volume
    parser.add_option("--generate_noisycyl",
                      action="store_true",
                      default=False,
                      help="Generate initial volume of noisy cylinder.")
    parser.add_option(
        "--boxsize",
        type="string",
        default="100,100,200",
        help=
        "String containing x , y, z dimensions (separated by comma) in pixels")
    parser.add_option("--rad",
                      type="int",
                      default=35,
                      help="Radius of initial volume in pixels")

    # generate 2D mask
    parser.add_option("--generate_mask",
                      action="store_true",
                      default=False,
                      help="Generate 2D rectangular mask.")
    parser.add_option(
        "--masksize",
        type="string",
        default="200,200",
        help=
        "String containing x and y dimensions (separated by comma) in pixels")
    parser.add_option("--maskwidth",
                      type="int",
                      default=60,
                      help="Width of rectangular mask")

    # Apply 2D alignment parameters to input stack and output new images to output stack
    parser.add_option(
        "--applyparams",
        action="store_true",
        default=False,
        help=
        "Apply the centering parameters to input stack, normalize using average and standard deviation outside the mask, and output the new images to output stack"
    )

    # Generate run script
    parser.add_option("--generate_script",
                      action="store_true",
                      default=False,
                      help="Generate script for helicon run through example")
    parser.add_option("--filename",
                      type="string",
                      default="runhelicon",
                      help="Name of run script to generate")
    parser.add_option("--seg_ny",
                      type="int",
                      default=180,
                      help="y-dimension of segment used for refinement")
    parser.add_option(
        "--ptcl_dist",
        type="int",
        default=15,
        help=
        "Distance in pixels between adjacent segments windowed from same filament"
    )
    parser.add_option(
        "--fract",
        type="float",
        default=0.35,
        help="Fraction of the volume used for applying helical symmetry.")

    (options, args) = parser.parse_args()
    if len(args) > 3:
        sxprint("usage: " + usage)
        sxprint("Please run '" + progname + " -h' for detailed options")
        ERROR(
            "Invalid number of parameters. Please see usage information above."
        )
        return

    else:
        if options.generate_script:
            generate_runscript(options.filename, options.seg_ny,
                               options.ptcl_dist, options.fract)

        if options.generate_micrograph:
            if options.apix <= 0:
                ERROR("Please enter pixel size.")
                return

            generate_helimic(args[0], args[1], options.apix, options.CTF,
                             options.Cs, options.voltage, options.ac,
                             options.nonoise, options.rand_seed)

        if options.generate_noisycyl:

            from sp_utilities import model_cylinder, model_gauss_noise
            outvol = args[0]
            boxdims = options.boxsize.split(',')

            if len(boxdims) < 1 or len(boxdims) > 3:
                ERROR(
                    "Enter box size as string containing x , y, z dimensions (separated by comma) in pixels. E.g.: --boxsize=\'100,100,200\'"
                )
                return

            nx = int(boxdims[0])

            if len(boxdims) == 1:
                ny = nx
                nz = nx
            else:
                ny = int(boxdims[1])
                if len(boxdims) == 3:
                    nz = int(boxdims[2])

            (model_cylinder(options.rad, nx, ny, nz) *
             model_gauss_noise(1.0, nx, ny, nz)).write_image(outvol)

        if options.generate_mask:
            from sp_utilities import model_blank, pad
            outvol = args[0]
            maskdims = options.masksize.split(',')

            if len(maskdims) < 1 or len(maskdims) > 2:
                ERROR(
                    "Enter box size as string containing x , y dimensions (separated by comma) in pixels. E.g.: --boxsize=\'200,200\'"
                )
                return

            nx = int(maskdims[0])

            if len(maskdims) == 1:
                ny = nx
            else:
                ny = int(maskdims[1])

            mask = pad(model_blank(options.maskwidth, ny, 1, 1.0), nx, ny, 1,
                       0.0)
            mask.write_image(outvol)

        if options.applyparams:
            from sp_utilities import get_im, get_params2D, set_params2D
            from sp_fundamentals import cyclic_shift
            stack = args[0]
            newstack = args[1]
            mask = get_im(args[2])
            nima = EMUtil.get_image_count(stack)
            for im in range(nima):
                prj = get_im(stack, im)
                alpha, sx, sy, mirror, scale = get_params2D(prj)
                prj = cyclic_shift(prj, int(sx))
                set_params2D(prj, [0.0, 0., 0.0, 0, 1])
                stat = Util.infomask(prj, mask, False)
                prj = (prj - stat[0]) / stat[1]
                ctf_params = prj.get_attr("ctf")
                prj.set_attr('ctf_applied', 0)
                prj.write_image(newstack, im)
Exemplo n.º 21
0
emnumpy2 = EMNumPy()
bigbuffer = emnumpy2.register_numpy_to_emdata(buffer)

# bigbuffer = EMNumPy.numpy2em(buffer)

if (Blockdata["myid_on_node"] == 0):
    #  read data on process 0 of each node
    #print "  READING DATA FIRST :",Blockdata["myid"],Blockdata["stack_ali2d"],len(plist)
    for i in range(nimastack):
        bigbuffer.insert_clip(data[i], (0, 0, i))

mpi.mpi_barrier(mpi.MPI_COMM_WORLD)
alldata = [None] * nimastack
emnumpy3 = [None] * nimastack

msk = sp_utilities.model_blank(target_nx, target_nx, 1, 1)
# for i in range(nimastack):
#     pointer_location = base_ptr + i*size_of_one_image*disp_unit
#     img_buffer  = np.frombuffer(np.core.multiarray.int_asbuffer(pointer_location, size_of_one_image*disp_unit), dtype = 'f4')
#     img_buffer  = img_buffer.reshape(target_nx, target_nx)
#     emnumpy3[i] = EMNumPy()
#     alldata[i]  = emnumpy3[i].register_numpy_to_emdata(img_buffer)

for i in range(nimastack):
    newpoint = base_ptr + i * size_of_one_image * disp_unit
    pointer_location = ctypes.cast(
        newpoint, ctypes.POINTER(ctypes.c_int * size_of_one_image))
    img_buffer = numpy.frombuffer(pointer_location.contents, dtype="f4")
    img_buffer = img_buffer.reshape(target_nx, target_nx)
    emnumpy3[i] = EMNumPy()
    alldata[i] = emnumpy3[i].register_numpy_to_emdata(img_buffer)
Exemplo n.º 22
0
def main():

    progname = os.path.basename(sys.argv[0])
    usage = progname + " proj_stack output_averages --MPI"
    parser = OptionParser(usage, version=SPARXVERSION)

    parser.add_option("--img_per_group",
                      type="int",
                      default=100,
                      help="number of images per group")
    parser.add_option("--radius",
                      type="int",
                      default=-1,
                      help="radius for alignment")
    parser.add_option(
        "--xr",
        type="string",
        default="2 1",
        help="range for translation search in x direction, search is +/xr")
    parser.add_option(
        "--yr",
        type="string",
        default="-1",
        help=
        "range for translation search in y direction, search is +/yr (default = same as xr)"
    )
    parser.add_option(
        "--ts",
        type="string",
        default="1 0.5",
        help=
        "step size of the translation search in both directions, search is -xr, -xr+ts, 0, xr-ts, xr, can be fractional"
    )
    parser.add_option(
        "--iter",
        type="int",
        default=30,
        help="number of iterations within alignment (default = 30)")
    parser.add_option(
        "--num_ali",
        type="int",
        default=5,
        help="number of alignments performed for stability (default = 5)")
    parser.add_option("--thld_err",
                      type="float",
                      default=1.0,
                      help="threshold of pixel error (default = 1.732)")
    parser.add_option(
        "--grouping",
        type="string",
        default="GRP",
        help=
        "do grouping of projections: PPR - per projection, GRP - different size groups, exclusive (default), GEV - grouping equal size"
    )
    parser.add_option(
        "--delta",
        type="float",
        default=-1.0,
        help="angular step for reference projections (required for GEV method)"
    )
    parser.add_option(
        "--fl",
        type="float",
        default=0.3,
        help="cut-off frequency of hyperbolic tangent low-pass Fourier filter")
    parser.add_option(
        "--aa",
        type="float",
        default=0.2,
        help="fall-off of hyperbolic tangent low-pass Fourier filter")
    parser.add_option("--CTF",
                      action="store_true",
                      default=False,
                      help="Consider CTF correction during the alignment ")
    parser.add_option("--MPI",
                      action="store_true",
                      default=False,
                      help="use MPI version")

    (options, args) = parser.parse_args()

    myid = mpi.mpi_comm_rank(MPI_COMM_WORLD)
    number_of_proc = mpi.mpi_comm_size(MPI_COMM_WORLD)
    main_node = 0

    if len(args) == 2:
        stack = args[0]
        outdir = args[1]
    else:
        sp_global_def.ERROR("Incomplete list of arguments",
                            "sxproj_stability.main",
                            1,
                            myid=myid)
        return
    if not options.MPI:
        sp_global_def.ERROR("Non-MPI not supported!",
                            "sxproj_stability.main",
                            1,
                            myid=myid)
        return

    if sp_global_def.CACHE_DISABLE:
        from sp_utilities import disable_bdb_cache
        disable_bdb_cache()
    sp_global_def.BATCH = True

    img_per_grp = options.img_per_group
    radius = options.radius
    ite = options.iter
    num_ali = options.num_ali
    thld_err = options.thld_err

    xrng = get_input_from_string(options.xr)
    if options.yr == "-1":
        yrng = xrng
    else:
        yrng = get_input_from_string(options.yr)

    step = get_input_from_string(options.ts)

    if myid == main_node:
        nima = EMUtil.get_image_count(stack)
        img = get_image(stack)
        nx = img.get_xsize()
        ny = img.get_ysize()
    else:
        nima = 0
        nx = 0
        ny = 0
    nima = bcast_number_to_all(nima)
    nx = bcast_number_to_all(nx)
    ny = bcast_number_to_all(ny)
    if radius == -1: radius = nx / 2 - 2
    mask = model_circle(radius, nx, nx)

    st = time()
    if options.grouping == "GRP":
        if myid == main_node:
            sxprint("  A  ", myid, "  ", time() - st)
            proj_attr = EMUtil.get_all_attributes(stack, "xform.projection")
            proj_params = []
            for i in range(nima):
                dp = proj_attr[i].get_params("spider")
                phi, theta, psi, s2x, s2y = dp["phi"], dp["theta"], dp[
                    "psi"], -dp["tx"], -dp["ty"]
                proj_params.append([phi, theta, psi, s2x, s2y])

            # Here is where the grouping is done, I didn't put enough annotation in the group_proj_by_phitheta,
            # So I will briefly explain it here
            # proj_list  : Returns a list of list of particle numbers, each list contains img_per_grp particle numbers
            #              except for the last one. Depending on the number of particles left, they will either form a
            #              group or append themselves to the last group
            # angle_list : Also returns a list of list, each list contains three numbers (phi, theta, delta), (phi,
            #              theta) is the projection angle of the center of the group, delta is the range of this group
            # mirror_list: Also returns a list of list, each list contains img_per_grp True or False, which indicates
            #              whether it should take mirror position.
            # In this program angle_list and mirror list are not of interest.

            proj_list_all, angle_list, mirror_list = group_proj_by_phitheta(
                proj_params, img_per_grp=img_per_grp)
            del proj_params
            sxprint("  B  number of groups  ", myid, "  ", len(proj_list_all),
                    time() - st)
        mpi_barrier(MPI_COMM_WORLD)

        # Number of groups, actually there could be one or two more groups, since the size of the remaining group varies
        # we will simply assign them to main node.
        n_grp = nima / img_per_grp - 1

        # Divide proj_list_all equally to all nodes, and becomes proj_list
        proj_list = []
        for i in range(n_grp):
            proc_to_stay = i % number_of_proc
            if proc_to_stay == main_node:
                if myid == main_node: proj_list.append(proj_list_all[i])
            elif myid == main_node:
                mpi_send(len(proj_list_all[i]), 1, MPI_INT, proc_to_stay,
                         SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
                mpi_send(proj_list_all[i], len(proj_list_all[i]), MPI_INT,
                         proc_to_stay, SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
            elif myid == proc_to_stay:
                img_per_grp = mpi_recv(1, MPI_INT, main_node,
                                       SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
                img_per_grp = int(img_per_grp[0])
                temp = mpi_recv(img_per_grp, MPI_INT, main_node,
                                SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
                proj_list.append(list(map(int, temp)))
                del temp
            mpi_barrier(MPI_COMM_WORLD)
        sxprint("  C  ", myid, "  ", time() - st)
        if myid == main_node:
            # Assign the remaining groups to main_node
            for i in range(n_grp, len(proj_list_all)):
                proj_list.append(proj_list_all[i])
            del proj_list_all, angle_list, mirror_list

    #   Compute stability per projection projection direction, equal number assigned, thus overlaps
    elif options.grouping == "GEV":

        if options.delta == -1.0:
            ERROR(
                "Angular step for reference projections is required for GEV method"
            )
            return

        from sp_utilities import even_angles, nearestk_to_refdir, getvec
        refproj = even_angles(options.delta)
        img_begin, img_end = MPI_start_end(len(refproj), number_of_proc, myid)
        # Now each processor keeps its own share of reference projections
        refprojdir = refproj[img_begin:img_end]
        del refproj

        ref_ang = [0.0] * (len(refprojdir) * 2)
        for i in range(len(refprojdir)):
            ref_ang[i * 2] = refprojdir[0][0]
            ref_ang[i * 2 + 1] = refprojdir[0][1] + i * 0.1

        sxprint("  A  ", myid, "  ", time() - st)
        proj_attr = EMUtil.get_all_attributes(stack, "xform.projection")
        #  the solution below is very slow, do not use it unless there is a problem with the i/O
        """
		for i in xrange(number_of_proc):
			if myid == i:
				proj_attr = EMUtil.get_all_attributes(stack, "xform.projection")
			mpi_barrier(MPI_COMM_WORLD)
		"""
        sxprint("  B  ", myid, "  ", time() - st)

        proj_ang = [0.0] * (nima * 2)
        for i in range(nima):
            dp = proj_attr[i].get_params("spider")
            proj_ang[i * 2] = dp["phi"]
            proj_ang[i * 2 + 1] = dp["theta"]
        sxprint("  C  ", myid, "  ", time() - st)
        asi = Util.nearestk_to_refdir(proj_ang, ref_ang, img_per_grp)
        del proj_ang, ref_ang
        proj_list = []
        for i in range(len(refprojdir)):
            proj_list.append(asi[i * img_per_grp:(i + 1) * img_per_grp])
        del asi
        sxprint("  D  ", myid, "  ", time() - st)
        #from sys import exit
        #exit()

    #   Compute stability per projection
    elif options.grouping == "PPR":
        sxprint("  A  ", myid, "  ", time() - st)
        proj_attr = EMUtil.get_all_attributes(stack, "xform.projection")
        sxprint("  B  ", myid, "  ", time() - st)
        proj_params = []
        for i in range(nima):
            dp = proj_attr[i].get_params("spider")
            phi, theta, psi, s2x, s2y = dp["phi"], dp["theta"], dp[
                "psi"], -dp["tx"], -dp["ty"]
            proj_params.append([phi, theta, psi, s2x, s2y])
        img_begin, img_end = MPI_start_end(nima, number_of_proc, myid)
        sxprint("  C  ", myid, "  ", time() - st)
        from sp_utilities import nearest_proj
        proj_list, mirror_list = nearest_proj(
            proj_params, img_per_grp,
            list(range(img_begin, img_begin + 1)))  #range(img_begin, img_end))
        refprojdir = proj_params[img_begin:img_end]
        del proj_params, mirror_list
        sxprint("  D  ", myid, "  ", time() - st)

    else:
        ERROR("Incorrect projection grouping option")
        return

    ###########################################################################################################
    # Begin stability test
    from sp_utilities import get_params_proj, read_text_file
    #if myid == 0:
    #	from utilities import read_text_file
    #	proj_list[0] = map(int, read_text_file("lggrpp0.txt"))

    from sp_utilities import model_blank
    aveList = [model_blank(nx, ny)] * len(proj_list)
    if options.grouping == "GRP":
        refprojdir = [[0.0, 0.0, -1.0]] * len(proj_list)
    for i in range(len(proj_list)):
        sxprint("  E  ", myid, "  ", time() - st)
        class_data = EMData.read_images(stack, proj_list[i])
        #print "  R  ",myid,"  ",time()-st
        if options.CTF:
            from sp_filter import filt_ctf
            for im in range(len(class_data)):  #  MEM LEAK!!
                atemp = class_data[im].copy()
                btemp = filt_ctf(atemp, atemp.get_attr("ctf"), binary=1)
                class_data[im] = btemp
                #class_data[im] = filt_ctf(class_data[im], class_data[im].get_attr("ctf"), binary=1)
        for im in class_data:
            try:
                t = im.get_attr(
                    "xform.align2d")  # if they are there, no need to set them!
            except:
                try:
                    t = im.get_attr("xform.projection")
                    d = t.get_params("spider")
                    set_params2D(im, [0.0, -d["tx"], -d["ty"], 0, 1.0])
                except:
                    set_params2D(im, [0.0, 0.0, 0.0, 0, 1.0])
        #print "  F  ",myid,"  ",time()-st
        # Here, we perform realignment num_ali times
        all_ali_params = []
        for j in range(num_ali):
            if (xrng[0] == 0.0 and yrng[0] == 0.0):
                avet = ali2d_ras(class_data,
                                 randomize=True,
                                 ir=1,
                                 ou=radius,
                                 rs=1,
                                 step=1.0,
                                 dst=90.0,
                                 maxit=ite,
                                 check_mirror=True,
                                 FH=options.fl,
                                 FF=options.aa)
            else:
                avet = within_group_refinement(class_data, mask, True, 1,
                                               radius, 1, xrng, yrng, step,
                                               90.0, ite, options.fl,
                                               options.aa)
            ali_params = []
            for im in range(len(class_data)):
                alpha, sx, sy, mirror, scale = get_params2D(class_data[im])
                ali_params.extend([alpha, sx, sy, mirror])
            all_ali_params.append(ali_params)
        #aveList[i] = avet
        #print "  G  ",myid,"  ",time()-st
        del ali_params
        # We determine the stability of this group here.
        # stable_set contains all particles deemed stable, it is a list of list
        # each list has two elements, the first is the pixel error, the second is the image number
        # stable_set is sorted based on pixel error
        #from utilities import write_text_file
        #write_text_file(all_ali_params, "all_ali_params%03d.txt"%myid)
        stable_set, mir_stab_rate, average_pix_err = multi_align_stability(
            all_ali_params, 0.0, 10000.0, thld_err, False, 2 * radius + 1)
        #print "  H  ",myid,"  ",time()-st
        if (len(stable_set) > 5):
            stable_set_id = []
            members = []
            pix_err = []
            # First put the stable members into attr 'members' and 'pix_err'
            for s in stable_set:
                # s[1] - number in this subset
                stable_set_id.append(s[1])
                # the original image number
                members.append(proj_list[i][s[1]])
                pix_err.append(s[0])
            # Then put the unstable members into attr 'members' and 'pix_err'
            from sp_fundamentals import rot_shift2D
            avet.to_zero()
            if options.grouping == "GRP":
                aphi = 0.0
                atht = 0.0
                vphi = 0.0
                vtht = 0.0
            l = -1
            for j in range(len(proj_list[i])):
                #  Here it will only work if stable_set_id is sorted in the increasing number, see how l progresses
                if j in stable_set_id:
                    l += 1
                    avet += rot_shift2D(class_data[j], stable_set[l][2][0],
                                        stable_set[l][2][1],
                                        stable_set[l][2][2],
                                        stable_set[l][2][3])
                    if options.grouping == "GRP":
                        phi, theta, psi, sxs, sy_s = get_params_proj(
                            class_data[j])
                        if (theta > 90.0):
                            phi = (phi + 540.0) % 360.0
                            theta = 180.0 - theta
                        aphi += phi
                        atht += theta
                        vphi += phi * phi
                        vtht += theta * theta
                else:
                    members.append(proj_list[i][j])
                    pix_err.append(99999.99)
            aveList[i] = avet.copy()
            if l > 1:
                l += 1
                aveList[i] /= l
                if options.grouping == "GRP":
                    aphi /= l
                    atht /= l
                    vphi = (vphi - l * aphi * aphi) / l
                    vtht = (vtht - l * atht * atht) / l
                    from math import sqrt
                    refprojdir[i] = [
                        aphi, atht,
                        (sqrt(max(vphi, 0.0)) + sqrt(max(vtht, 0.0))) / 2.0
                    ]

            # Here more information has to be stored, PARTICULARLY WHAT IS THE REFERENCE DIRECTION
            aveList[i].set_attr('members', members)
            aveList[i].set_attr('refprojdir', refprojdir[i])
            aveList[i].set_attr('pixerr', pix_err)
        else:
            sxprint(" empty group ", i, refprojdir[i])
            aveList[i].set_attr('members', [-1])
            aveList[i].set_attr('refprojdir', refprojdir[i])
            aveList[i].set_attr('pixerr', [99999.])

    del class_data

    if myid == main_node:
        km = 0
        for i in range(number_of_proc):
            if i == main_node:
                for im in range(len(aveList)):
                    aveList[im].write_image(args[1], km)
                    km += 1
            else:
                nl = mpi_recv(1, MPI_INT, i, SPARX_MPI_TAG_UNIVERSAL,
                              MPI_COMM_WORLD)
                nl = int(nl[0])
                for im in range(nl):
                    ave = recv_EMData(i, im + i + 70000)
                    nm = mpi_recv(1, MPI_INT, i, SPARX_MPI_TAG_UNIVERSAL,
                                  MPI_COMM_WORLD)
                    nm = int(nm[0])
                    members = mpi_recv(nm, MPI_INT, i, SPARX_MPI_TAG_UNIVERSAL,
                                       MPI_COMM_WORLD)
                    ave.set_attr('members', list(map(int, members)))
                    members = mpi_recv(nm, MPI_FLOAT, i,
                                       SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
                    ave.set_attr('pixerr', list(map(float, members)))
                    members = mpi_recv(3, MPI_FLOAT, i,
                                       SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
                    ave.set_attr('refprojdir', list(map(float, members)))
                    ave.write_image(args[1], km)
                    km += 1
    else:
        mpi_send(len(aveList), 1, MPI_INT, main_node, SPARX_MPI_TAG_UNIVERSAL,
                 MPI_COMM_WORLD)
        for im in range(len(aveList)):
            send_EMData(aveList[im], main_node, im + myid + 70000)
            members = aveList[im].get_attr('members')
            mpi_send(len(members), 1, MPI_INT, main_node,
                     SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
            mpi_send(members, len(members), MPI_INT, main_node,
                     SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
            members = aveList[im].get_attr('pixerr')
            mpi_send(members, len(members), MPI_FLOAT, main_node,
                     SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
            try:
                members = aveList[im].get_attr('refprojdir')
                mpi_send(members, 3, MPI_FLOAT, main_node,
                         SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)
            except:
                mpi_send([-999.0, -999.0, -999.0], 3, MPI_FLOAT, main_node,
                         SPARX_MPI_TAG_UNIVERSAL, MPI_COMM_WORLD)

    sp_global_def.BATCH = False
    mpi_barrier(MPI_COMM_WORLD)
Exemplo n.º 23
0
def cml_open_proj(stack, ir, ou, lf, hf, dpsi=1):
    from sp_projection import cml_sinogram
    from sp_utilities import model_circle, get_params_proj, model_blank, get_im
    from sp_fundamentals import fftip
    from sp_filter import filt_tanh

    # number of projections
    if type(stack) == type(""): nprj = EMUtil.get_image_count(stack)
    else: nprj = len(stack)
    Prj = []  # list of projections
    Ori = [
        -1
    ] * 4 * nprj  # orientation intial (phi, theta, psi, index) for each projection

    for i in range(nprj):
        image = get_im(stack, i)

        # read initial angles if given
        try:
            Ori[4 * i], Ori[4 * i +
                            1], Ori[4 * i +
                                    2], s2x, s2y = get_params_proj(image)
        except:
            pass

        if (i == 0):
            nx = image.get_xsize()
            if (ou < 1): ou = nx // 2 - 1
            diameter = int(2 * ou)
            mask2D = model_circle(ou, nx, nx)
            if ir > 0: mask2D -= model_circle(ir, nx, nx)

        # normalize under the mask
        [mean_a, sigma, imin, imax] = Util.infomask(image, mask2D, True)
        image -= mean_a
        Util.mul_scalar(image, 1.0 / sigma)
        Util.mul_img(image, mask2D)

        # sinogram
        sino = cml_sinogram(image, diameter, dpsi)

        # prepare the cut positions in order to filter (lf: low freq; hf: high freq)
        ihf = min(int(2 * hf * diameter), diameter + (diameter + 1) % 2)
        ihf = ihf + (ihf + 1) % 2  # index ihf must be odd to take the img part
        ilf = max(int(2 * lf * diameter), 0)
        ilf = ilf + ilf % 2  # index ilf must be even to fall in the real part
        bdf = ihf - ilf + 1

        # process lines
        nxe = sino.get_xsize()
        nye = sino.get_ysize()
        prj = model_blank(bdf, 2 * nye)
        pp = model_blank(nxe, 2 * nye)
        for li in range(nye):
            # get the line li
            line = Util.window(sino, nxe, 1, 1, 0, li - nye // 2, 0)
            # u2 (not improve the results)
            #line = filt_tanh(line, ou / float(nx), ou / float(nx))
            # normalize this line
            [mean_l, sigma_l, imin, imax] = Util.infomask(line, None, True)
            line = (line - mean_l) / sigma_l
            # fft
            fftip(line)
            # filter (cut part of coef) and create mirror line
            Util.cml_prepare_line(prj, line, ilf, ihf, li, nye)

        # store the projection
        Prj.append(prj)

    return Prj, Ori
Exemplo n.º 24
0
def helicalshiftali_MPI(stack,
                        maskfile=None,
                        maxit=100,
                        CTF=False,
                        snr=1.0,
                        Fourvar=False,
                        search_rng=-1):

    nproc = mpi.mpi_comm_size(mpi.MPI_COMM_WORLD)
    myid = mpi.mpi_comm_rank(mpi.MPI_COMM_WORLD)
    main_node = 0

    ftp = file_type(stack)

    if myid == main_node:
        print_begin_msg("helical-shiftali_MPI")

    max_iter = int(maxit)
    if (myid == main_node):
        infils = EMUtil.get_all_attributes(stack, "filament")
        ptlcoords = EMUtil.get_all_attributes(stack, 'ptcl_source_coord')
        filaments = ordersegments(infils, ptlcoords)
        total_nfils = len(filaments)
        inidl = [0] * total_nfils
        for i in range(total_nfils):
            inidl[i] = len(filaments[i])
        linidl = sum(inidl)
        nima = linidl
        tfilaments = []
        for i in range(total_nfils):
            tfilaments += filaments[i]
        del filaments
    else:
        total_nfils = 0
        linidl = 0
    total_nfils = bcast_number_to_all(total_nfils, source_node=main_node)
    if myid != main_node:
        inidl = [-1] * total_nfils
    inidl = bcast_list_to_all(inidl, myid, source_node=main_node)
    linidl = bcast_number_to_all(linidl, source_node=main_node)
    if myid != main_node:
        tfilaments = [-1] * linidl
    tfilaments = bcast_list_to_all(tfilaments, myid, source_node=main_node)
    filaments = []
    iendi = 0
    for i in range(total_nfils):
        isti = iendi
        iendi = isti + inidl[i]
        filaments.append(tfilaments[isti:iendi])
    del tfilaments, inidl

    if myid == main_node:
        print_msg("total number of filaments: %d" % total_nfils)
    if total_nfils < nproc:
        ERROR(
            'number of CPUs (%i) is larger than the number of filaments (%i), please reduce the number of CPUs used'
            % (nproc, total_nfils),
            myid=myid)

    #  balanced load
    temp = chunks_distribution([[len(filaments[i]), i]
                                for i in range(len(filaments))],
                               nproc)[myid:myid + 1][0]
    filaments = [filaments[temp[i][1]] for i in range(len(temp))]
    nfils = len(filaments)

    #filaments = [[0,1]]
    #print "filaments",filaments
    list_of_particles = []
    indcs = []
    k = 0
    for i in range(nfils):
        list_of_particles += filaments[i]
        k1 = k + len(filaments[i])
        indcs.append([k, k1])
        k = k1
    data = EMData.read_images(stack, list_of_particles)
    ldata = len(data)
    sxprint("ldata=", ldata)
    nx = data[0].get_xsize()
    ny = data[0].get_ysize()
    if maskfile == None:
        mrad = min(nx, ny) // 2 - 2
        mask = pad(model_blank(2 * mrad + 1, ny, 1, 1.0), nx, ny, 1, 0.0)
    else:
        mask = get_im(maskfile)

    # apply initial xform.align2d parameters stored in header
    init_params = []
    for im in range(ldata):
        t = data[im].get_attr('xform.align2d')
        init_params.append(t)
        p = t.get_params("2d")
        data[im] = rot_shift2D(data[im], p['alpha'], p['tx'], p['ty'],
                               p['mirror'], p['scale'])

    if CTF:
        from sp_filter import filt_ctf
        from sp_morphology import ctf_img
        ctf_abs_sum = EMData(nx, ny, 1, False)
        ctf_2_sum = EMData(nx, ny, 1, False)
    else:
        ctf_2_sum = None
        ctf_abs_sum = None

    from sp_utilities import info

    for im in range(ldata):
        data[im].set_attr('ID', list_of_particles[im])
        st = Util.infomask(data[im], mask, False)
        data[im] -= st[0]
        if CTF:
            ctf_params = data[im].get_attr("ctf")
            qctf = data[im].get_attr("ctf_applied")
            if qctf == 0:
                data[im] = filt_ctf(fft(data[im]), ctf_params)
                data[im].set_attr('ctf_applied', 1)
            elif qctf != 1:
                ERROR('Incorrectly set qctf flag', myid=myid)
            ctfimg = ctf_img(nx, ctf_params, ny=ny)
            Util.add_img2(ctf_2_sum, ctfimg)
            Util.add_img_abs(ctf_abs_sum, ctfimg)
        else:
            data[im] = fft(data[im])

    del list_of_particles

    if CTF:
        reduce_EMData_to_root(ctf_2_sum, myid, main_node)
        reduce_EMData_to_root(ctf_abs_sum, myid, main_node)
    if CTF:
        if myid != main_node:
            del ctf_2_sum
            del ctf_abs_sum
        else:
            temp = EMData(nx, ny, 1, False)
            tsnr = 1. / snr
            for i in range(0, nx + 2, 2):
                for j in range(ny):
                    temp.set_value_at(i, j, tsnr)
                    temp.set_value_at(i + 1, j, 0.0)
            #info(ctf_2_sum)
            Util.add_img(ctf_2_sum, temp)
            #info(ctf_2_sum)
            del temp

    total_iter = 0
    shift_x = [0.0] * ldata

    for Iter in range(max_iter):
        if myid == main_node:
            start_time = time()
            print_msg("Iteration #%4d\n" % (total_iter))
        total_iter += 1
        avg = EMData(nx, ny, 1, False)
        for im in range(ldata):
            Util.add_img(avg, fshift(data[im], shift_x[im]))

        reduce_EMData_to_root(avg, myid, main_node)

        if myid == main_node:
            if CTF: tavg = Util.divn_filter(avg, ctf_2_sum)
            else: tavg = Util.mult_scalar(avg, 1.0 / float(nima))
        else:
            tavg = model_blank(nx, ny)

        if Fourvar:
            bcast_EMData_to_all(tavg, myid, main_node)
            vav, rvar = varf2d_MPI(myid, data, tavg, mask, "a", CTF)

        if myid == main_node:
            if Fourvar:
                tavg = fft(Util.divn_img(fft(tavg), vav))
                vav_r = Util.pack_complex_to_real(vav)
            # normalize and mask tavg in real space
            tavg = fft(tavg)
            stat = Util.infomask(tavg, mask, False)
            tavg -= stat[0]
            Util.mul_img(tavg, mask)
            tavg.write_image("tavg.hdf", Iter)
            # For testing purposes: shift tavg to some random place and see if the centering is still correct
            #tavg = rot_shift3D(tavg,sx=3,sy=-4)

        if Fourvar: del vav
        bcast_EMData_to_all(tavg, myid, main_node)
        tavg = fft(tavg)

        sx_sum = 0.0
        nxc = nx // 2

        for ifil in range(nfils):
            """
			# Calculate filament average
			avg = EMData(nx, ny, 1, False)
			filnima = 0
			for im in xrange(indcs[ifil][0], indcs[ifil][1]):
				Util.add_img(avg, data[im])
				filnima += 1
			tavg = Util.mult_scalar(avg, 1.0/float(filnima))
			"""
            # Calculate 1D ccf between each segment and filament average
            nsegms = indcs[ifil][1] - indcs[ifil][0]
            ctx = [None] * nsegms
            pcoords = [None] * nsegms
            for im in range(indcs[ifil][0], indcs[ifil][1]):
                ctx[im - indcs[ifil][0]] = Util.window(ccf(tavg, data[im]), nx,
                                                       1)
                pcoords[im - indcs[ifil][0]] = data[im].get_attr(
                    'ptcl_source_coord')
                #ctx[im-indcs[ifil][0]].write_image("ctx.hdf",im-indcs[ifil][0])
                #print "  CTX  ",myid,im,Util.infomask(ctx[im-indcs[ifil][0]], None, True)
            # search for best x-shift
            cents = nsegms // 2

            dst = sqrt(
                max((pcoords[cents][0] - pcoords[0][0])**2 +
                    (pcoords[cents][1] - pcoords[0][1])**2,
                    (pcoords[cents][0] - pcoords[-1][0])**2 +
                    (pcoords[cents][1] - pcoords[-1][1])**2))
            maxincline = atan2(ny // 2 - 2 - float(search_rng), dst)
            kang = int(dst * tan(maxincline) + 0.5)
            #print  "  settings ",nsegms,cents,dst,search_rng,maxincline,kang

            # ## C code for alignment. @ming
            results = [0.0] * 3
            results = Util.helixshiftali(ctx, pcoords, nsegms, maxincline,
                                         kang, search_rng, nxc)
            sib = int(results[0])
            bang = results[1]
            qm = results[2]
            #print qm, sib, bang

            # qm = -1.e23
            #
            # 			for six in xrange(-search_rng, search_rng+1,1):
            # 				q0 = ctx[cents].get_value_at(six+nxc)
            # 				for incline in xrange(kang+1):
            # 					qt = q0
            # 					qu = q0
            # 					if(kang>0):  tang = tan(maxincline/kang*incline)
            # 					else:        tang = 0.0
            # 					for kim in xrange(cents+1,nsegms):
            # 						dst = sqrt((pcoords[cents][0] - pcoords[kim][0])**2 + (pcoords[cents][1] - pcoords[kim][1])**2)
            # 						xl = dst*tang+six+nxc
            # 						ixl = int(xl)
            # 						dxl = xl - ixl
            # 						#print "  A  ", ifil,six,incline,kim,xl,ixl,dxl
            # 						qt += (1.0-dxl)*ctx[kim].get_value_at(ixl) + dxl*ctx[kim].get_value_at(ixl+1)
            # 						xl = -dst*tang+six+nxc
            # 						ixl = int(xl)
            # 						dxl = xl - ixl
            # 						qu += (1.0-dxl)*ctx[kim].get_value_at(ixl) + dxl*ctx[kim].get_value_at(ixl+1)
            # 					for kim in xrange(cents):
            # 						dst = sqrt((pcoords[cents][0] - pcoords[kim][0])**2 + (pcoords[cents][1] - pcoords[kim][1])**2)
            # 						xl = -dst*tang+six+nxc
            # 						ixl = int(xl)
            # 						dxl = xl - ixl
            # 						qt += (1.0-dxl)*ctx[kim].get_value_at(ixl) + dxl*ctx[kim].get_value_at(ixl+1)
            # 						xl =  dst*tang+six+nxc
            # 						ixl = int(xl)
            # 						dxl = xl - ixl
            # 						qu += (1.0-dxl)*ctx[kim].get_value_at(ixl) + dxl*ctx[kim].get_value_at(ixl+1)
            # 					if( qt > qm ):
            # 						qm = qt
            # 						sib = six
            # 						bang = tang
            # 					if( qu > qm ):
            # 						qm = qu
            # 						sib = six
            # 						bang = -tang
            #if incline == 0:  print  "incline = 0  ",six,tang,qt,qu
            #print qm,six,sib,bang
            #print " got results   ",indcs[ifil][0], indcs[ifil][1], ifil,myid,qm,sib,tang,bang,len(ctx),Util.infomask(ctx[0], None, True)
            for im in range(indcs[ifil][0], indcs[ifil][1]):
                kim = im - indcs[ifil][0]
                dst = sqrt((pcoords[cents][0] - pcoords[kim][0])**2 +
                           (pcoords[cents][1] - pcoords[kim][1])**2)
                if (kim < cents): xl = -dst * bang + sib
                else: xl = dst * bang + sib
                shift_x[im] = xl

            # Average shift
            sx_sum += shift_x[indcs[ifil][0] + cents]

        # #print myid,sx_sum,total_nfils
        sx_sum = mpi.mpi_reduce(sx_sum, 1, mpi.MPI_FLOAT, mpi.MPI_SUM,
                                main_node, mpi.MPI_COMM_WORLD)
        if myid == main_node:
            sx_sum = float(sx_sum[0]) / total_nfils
            print_msg("Average shift  %6.2f\n" % (sx_sum))
        else:
            sx_sum = 0.0
        sx_sum = 0.0
        sx_sum = bcast_number_to_all(sx_sum, source_node=main_node)
        for im in range(ldata):
            shift_x[im] -= sx_sum
            #print  "   %3d  %6.3f"%(im,shift_x[im])
        #exit()

    # combine shifts found with the original parameters
    for im in range(ldata):
        t1 = Transform()
        ##import random
        ##shix=random.randint(-10, 10)
        ##t1.set_params({"type":"2D","tx":shix})
        t1.set_params({"type": "2D", "tx": shift_x[im]})
        # combine t0 and t1
        tt = t1 * init_params[im]
        data[im].set_attr("xform.align2d", tt)
    # write out headers and STOP, under MPI writing has to be done sequentially
    mpi.mpi_barrier(mpi.MPI_COMM_WORLD)
    par_str = ["xform.align2d", "ID"]
    if myid == main_node:
        from sp_utilities import file_type
        if (file_type(stack) == "bdb"):
            from sp_utilities import recv_attr_dict_bdb
            recv_attr_dict_bdb(main_node, stack, data, par_str, 0, ldata,
                               nproc)
        else:
            from sp_utilities import recv_attr_dict
            recv_attr_dict(main_node, stack, data, par_str, 0, ldata, nproc)
    else:
        send_attr_dict(main_node, data, par_str, 0, ldata)
    if myid == main_node: print_end_msg("helical-shiftali_MPI")
Exemplo n.º 25
0
def main():
    arglist = []
    for arg in sys.argv:
        arglist.append(arg)
    progname = os.path.basename(arglist[0])
    usage = progname + """ firstvolume  secondvolume  maskfile  directory  --prefix  --wn  --step  --cutoff  --radius  --fsc  --res_overall  --out_ang_res  --apix  --MPI

	Compute local resolution in real space within area outlined by the maskfile and within regions wn x wn x wn
	"""
    parser = optparse.OptionParser(usage, version=sp_global_def.SPARXVERSION)

    parser.add_option("--prefix",
                      type="str",
                      default='localres',
                      help="Prefix for the output files. (default localres)")
    parser.add_option(
        "--wn",
        type="int",
        default=7,
        help=
        "Size of window within which local real-space FSC is computed. (default 7)"
    )
    parser.add_option(
        "--step",
        type="float",
        default=1.0,
        help="Shell step in Fourier size in pixels. (default 1.0)")
    parser.add_option("--cutoff",
                      type="float",
                      default=0.143,
                      help="Resolution cut-off for FSC. (default 0.143)")
    parser.add_option(
        "--radius",
        type="int",
        default=-1,
        help=
        "If there is no maskfile, sphere with r=radius will be used. By default, the radius is nx/2-wn (default -1)"
    )
    parser.add_option(
        "--fsc",
        type="string",
        default=None,
        help=
        "Save overall FSC curve (might be truncated). By default, the program does not save the FSC curve. (default none)"
    )
    parser.add_option(
        "--res_overall",
        type="float",
        default=-1.0,
        help=
        "Overall resolution at the cutoff level estimated by the user [abs units]. (default None)"
    )
    parser.add_option(
        "--out_ang_res",
        action="store_true",
        default=False,
        help=
        "Additionally creates a local resolution file in Angstroms. (default False)"
    )
    parser.add_option(
        "--apix",
        type="float",
        default=1.0,
        help=
        "Pixel size in Angstrom. Effective only with --out_ang_res options. (default 1.0)"
    )
    parser.add_option("--MPI",
                      action="store_true",
                      default=False,
                      help="Use MPI version.")

    (options, args) = parser.parse_args(arglist[1:])

    if len(args) < 3 or len(args) > 4:
        sxprint("Usage: " + usage)
        ERROR(
            "Invalid number of parameters used. Please see usage information above."
        )
        return

    if sp_global_def.CACHE_DISABLE:
        sp_utilities.disable_bdb_cache()

    res_overall = options.res_overall

    if options.MPI:

        number_of_proc = mpi.mpi_comm_size(mpi.MPI_COMM_WORLD)
        myid = mpi.mpi_comm_rank(mpi.MPI_COMM_WORLD)
        main_node = 0
        sp_global_def.MPI = True
        cutoff = options.cutoff

        nk = int(options.wn)

        if (myid == main_node):
            #print sys.argv
            vi = sp_utilities.get_im(sys.argv[1])
            ui = sp_utilities.get_im(sys.argv[2])

            nx = vi.get_xsize()
            ny = vi.get_ysize()
            nz = vi.get_zsize()
            dis = [nx, ny, nz]
        else:
            dis = [0, 0, 0, 0]

        sp_global_def.BATCH = True

        dis = sp_utilities.bcast_list_to_all(dis, myid, source_node=main_node)

        if (myid != main_node):
            nx = int(dis[0])
            ny = int(dis[1])
            nz = int(dis[2])

            vi = sp_utilities.model_blank(nx, ny, nz)
            ui = sp_utilities.model_blank(nx, ny, nz)

        if len(args) == 3:
            m = sp_utilities.model_circle((min(nx, ny, nz) - nk) // 2, nx, ny,
                                          nz)
            outdir = args[2]

        elif len(args) == 4:
            if (myid == main_node):
                m = sp_morphology.binarize(sp_utilities.get_im(args[2]), 0.5)
            else:
                m = sp_utilities.model_blank(nx, ny, nz)
            outdir = args[3]
        if os.path.exists(outdir) and myid == 0:
            sp_global_def.ERROR('Output directory already exists!')
        elif myid == 0:
            os.makedirs(outdir)
        sp_global_def.write_command(outdir)
        sp_utilities.bcast_EMData_to_all(m, myid, main_node)
        """Multiline Comment0"""
        freqvol, resolut = sp_statistics.locres(vi, ui, m, nk, cutoff,
                                                options.step, myid, main_node,
                                                number_of_proc)

        if (myid == 0):
            # Remove outliers based on the Interquartile range
            output_volume(freqvol, resolut, options.apix, outdir,
                          options.prefix, options.fsc, options.out_ang_res, nx,
                          ny, nz, res_overall)

    else:
        cutoff = options.cutoff
        vi = sp_utilities.get_im(args[0])
        ui = sp_utilities.get_im(args[1])

        nn = vi.get_xsize()
        nx = nn
        ny = nn
        nz = nn
        nk = int(options.wn)

        if len(args) == 3:
            m = sp_utilities.model_circle((nn - nk) // 2, nn, nn, nn)
            outdir = args[2]

        elif len(args) == 4:
            m = sp_morphology.binarize(sp_utilities.get_im(args[2]), 0.5)
            outdir = args[3]
        if os.path.exists(outdir):
            sp_global_def.ERROR('Output directory already exists!')
        else:
            os.makedirs(outdir)
        sp_global_def.write_command(outdir)

        mc = sp_utilities.model_blank(nn, nn, nn, 1.0) - m

        vf = sp_fundamentals.fft(vi)
        uf = sp_fundamentals.fft(ui)
        """Multiline Comment1"""
        lp = int(nn / 2 / options.step + 0.5)
        step = 0.5 / lp

        freqvol = sp_utilities.model_blank(nn, nn, nn)
        resolut = []
        for i in range(1, lp):
            fl = step * i
            fh = fl + step
            #print(lp,i,step,fl,fh)
            v = sp_fundamentals.fft(sp_filter.filt_tophatb(vf, fl, fh))
            u = sp_fundamentals.fft(sp_filter.filt_tophatb(uf, fl, fh))
            tmp1 = EMAN2_cppwrap.Util.muln_img(v, v)
            tmp2 = EMAN2_cppwrap.Util.muln_img(u, u)

            do = EMAN2_cppwrap.Util.infomask(
                sp_morphology.square_root(
                    sp_morphology.threshold(
                        EMAN2_cppwrap.Util.muln_img(tmp1, tmp2))), m, True)[0]

            tmp3 = EMAN2_cppwrap.Util.muln_img(u, v)
            dp = EMAN2_cppwrap.Util.infomask(tmp3, m, True)[0]
            resolut.append([i, (fl + fh) / 2.0, dp / do])

            tmp1 = EMAN2_cppwrap.Util.box_convolution(tmp1, nk)
            tmp2 = EMAN2_cppwrap.Util.box_convolution(tmp2, nk)
            tmp3 = EMAN2_cppwrap.Util.box_convolution(tmp3, nk)

            EMAN2_cppwrap.Util.mul_img(tmp1, tmp2)

            tmp1 = sp_morphology.square_root(sp_morphology.threshold(tmp1))

            EMAN2_cppwrap.Util.mul_img(tmp1, m)
            EMAN2_cppwrap.Util.add_img(tmp1, mc)

            EMAN2_cppwrap.Util.mul_img(tmp3, m)
            EMAN2_cppwrap.Util.add_img(tmp3, mc)

            EMAN2_cppwrap.Util.div_img(tmp3, tmp1)

            EMAN2_cppwrap.Util.mul_img(tmp3, m)
            freq = (fl + fh) / 2.0
            bailout = True
            for x in range(nn):
                for y in range(nn):
                    for z in range(nn):
                        if (m.get_value_at(x, y, z) > 0.5):
                            if (freqvol.get_value_at(x, y, z) == 0.0):
                                if (tmp3.get_value_at(x, y, z) < cutoff):
                                    freqvol.set_value_at(x, y, z, freq)
                                    bailout = False
                                else:
                                    bailout = False
            if (bailout): break
        #print(len(resolut))
        # remove outliers
        output_volume(freqvol, resolut, options.apix, outdir, options.prefix,
                      options.fsc, options.out_ang_res, nx, ny, nz,
                      res_overall)