def generate_baseline_coordinates(layout, settings): """Generate baseline coordinates""" x, y = layout['x'], layout['y'] wavelength_m = 299792458.0 / settings['freq_hz'] mjd_start = settings['mjd_mid'] - (settings['obs_length_s'] / 2.0) / 86400.0 x, y, z = np.array(x), np.array(y), np.zeros_like(x) x_ecef, y_ecef, z_ecef = convert_enu_to_ecef(x, y, z, settings['lon'], settings['lat']) x_c, y_c, z_c = convert_enu_to_ecef([0.0], [0.0], [0.0], settings['lon'], settings['lat']) x_ecef -= x_c y_ecef -= y_c z_ecef -= z_c num_stations = x_ecef.shape[0] num_baselines = num_stations * (num_stations - 1) / 2 num_coords = settings['num_times'] * num_baselines uu = np.zeros(num_coords, dtype='f4') vv, ww = np.zeros_like(uu), np.zeros_like(uu) u = np.zeros(num_stations, dtype='f4') v, w = np.zeros_like(u), np.zeros_like(u) for i in range(settings['num_times']): mjd = mjd_start + (i * settings['interval_s'] + settings['interval_s'] / 2.0) / 86400.0 uu_, vv_, ww_ = evaluate_baseline_uvw(x_ecef, y_ecef, z_ecef, settings['ra'], settings['dec'], mjd) u, v, w = evaluate_station_uvw(x_ecef, y_ecef, z_ecef, settings['ra'], settings['dec'], mjd) uu[i * num_baselines: (i + 1) * num_baselines] = uu_ / wavelength_m vv[i * num_baselines: (i + 1) * num_baselines] = vv_ / wavelength_m ww[i * num_baselines: (i + 1) * num_baselines] = ww_ / wavelength_m return uu, vv, ww, u, w, v
def load_telescope(r_cut, station_d, lon, lat, plot_filename=None): # Load telescope model coords = np.loadtxt(join('v5.tm', 'layout.txt')) x, y, z = coords[:, 0], coords[:, 1], coords[:, 2] r = (x**2 + y**2)**0.5 x = x[np.where(r < r_cut)] y = y[np.where(r < r_cut)] z = z[np.where(r < r_cut)] num_stations = x.shape[0] if plot_filename: plot_telescope(x, y, r_cut, station_d=station_d, filename=plot_filename) x, y, z = convert_enu_to_ecef(x, y, z, lon, lat) return x, y, z
def gen_uvw_coords(self): """Generate uvw coordinates""" x, y, z = self.get_coords_enu() x, y, z = convert_enu_to_ecef(x, y, z, radians(self.lon_deg), radians(self.lat_deg), self.alt_m) num_stations = x.shape[0] num_baselines = num_stations * (num_stations - 1) // 2 n = num_baselines * self.num_times self.uu_m, self.vv_m, self.ww_m = np.zeros(n), np.zeros(n), np.zeros(n) ha_off = ((self.obs_length_h / 2) / 24) * (2 * pi) for i, ha in enumerate(np.linspace(-ha_off, ha_off, self.num_times)): uu_, vv_, ww_ = evaluate_baseline_uvw_ha_dec( x, y, z, ha - radians(self.lon_deg), radians(self.dec_deg)) self.uu_m[i * num_baselines: (i + 1) * num_baselines] = uu_ self.vv_m[i * num_baselines: (i + 1) * num_baselines] = vv_ self.ww_m[i * num_baselines: (i + 1) * num_baselines] = ww_ self.r_uv_m = (self.uu_m**2 + self.vv_m**2)**0.5
def gen_uvw_coords(self): """Generate uvw coordinates""" x, y, z = self.get_coords_enu() x, y, z = convert_enu_to_ecef(x, y, z, radians(self.lon_deg), radians(self.lat_deg), self.alt_m) num_stations = x.shape[0] num_baselines = num_stations * (num_stations - 1) // 2 n = num_baselines * self.num_times self.uu_m, self.vv_m, self.ww_m = np.zeros(n), np.zeros(n), np.zeros(n) ha_off = ((self.obs_length_h / 2) / 24) * (2 * pi) for i, ha in enumerate(np.linspace(-ha_off, ha_off, self.num_times)): uu_, vv_, ww_ = evaluate_baseline_uvw_ha_dec( x, y, z, ha - radians(self.lon_deg), radians(self.dec_deg)) self.uu_m[i * num_baselines:(i + 1) * num_baselines] = uu_ self.vv_m[i * num_baselines:(i + 1) * num_baselines] = vv_ self.ww_m[i * num_baselines:(i + 1) * num_baselines] = ww_ self.r_uv_m = (self.uu_m**2 + self.vv_m**2)**0.5
def generate_uv_coordinates( x, y, z, lon, lat, alt, ra, dec, num_times, num_baselines, mjd_start, dt_s, freq_hz, uv_cut_radius_wavelengths ): x, y, z = convert_enu_to_ecef(x, y, z, lon, lat, alt) uu, vv, ww = generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) wave_length = 299792458.0 / freq_hz uu /= wave_length vv /= wave_length ww /= wave_length # uv_r_cut = uv_cut_radius_wavelengths # uv_r = (uu ** 2 + vv ** 2) ** 0.5 # uv_sort_idx = numpy.argsort(uv_r) # uv_r = uv_r[uv_sort_idx] # uu = uu[uv_sort_idx] # vv = vv[uv_sort_idx] # ww = ww[uv_sort_idx] # i_uv_max = numpy.argmax(uv_r >= uv_r_cut) # uu = uu[:i_uv_max] # vv = vv[:i_uv_max] # ww = ww[:i_uv_max] uu = numpy.hstack((uu, -uu)) vv = numpy.hstack((vv, -vv)) ww = numpy.hstack((ww, -ww)) return uu, vv, ww
def generate_baseline_coords(layout, settings): x, y = layout['x'], layout['y'] z = numpy.zeros_like(x) wavelength_m = 299792458.0 / settings['freq_hz'] mjd_start = settings['mjd_mid'] - (settings['obs_length_s'] / 2.0) / 86400.0 x, y, z = numpy.array(x), numpy.array(y), numpy.zeros_like(x) x_ecef, y_ecef, z_ecef = pyuvwsim.convert_enu_to_ecef(x, y, z, settings['lon'], settings['lat']) num_stations = x_ecef.shape[0] num_baselines = num_stations * (num_stations - 1) / 2 num_coords = settings['num_times'] * num_baselines uu = numpy.zeros(num_coords, dtype='f4') vv, ww = numpy.zeros_like(uu), numpy.zeros_like(uu) for i in range(settings['num_times']): mjd = mjd_start + (i * settings['interval_s'] + settings['interval_s'] / 2.0) / 86400.0 uu_, vv_, ww_ = pyuvwsim.evaluate_baseline_uvw(x_ecef, y_ecef, z_ecef, settings['ra'], settings['dec'], mjd) uu[i * num_baselines: (i + 1) * num_baselines] = uu_ / wavelength_m vv[i * num_baselines: (i + 1) * num_baselines] = vv_ / wavelength_m ww[i * num_baselines: (i + 1) * num_baselines] = ww_ / wavelength_m return uu, vv, ww
def main(): out_dir = 'TEMP_0h' layouts = OrderedDict() layouts['v5'] = {'filename': join('v5.tm', 'layout.txt')} layouts['v5c'] = {'filename': join('v5c.tm', 'layout_enu_stations.txt')} station_radius_m = 40.0 / 2.0 freq_hz = 100.0e6 wave_length = 299792458.0 / freq_hz lon = radians(116.63128900) lat = radians(-26.69702400) ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 snapshot = True if snapshot: mjd_start = mjd_mid obs_length = 0.0 dt_s = 0.0 num_times = 1 else: obs_length = 4.0 * 3600.0 # seconds num_times = int(obs_length / (1 * 60.0)) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - (obs_length / 2.0) / (3600.0 * 24.0) # Create output directory and copy script ================================= if os.path.exists(out_dir): shutil.rmtree(out_dir) os.makedirs(out_dir) shutil.copy(__file__, join(out_dir, 'copy_' + os.path.basename(__file__))) # Load station coordinates & generate baseline coordinates ================ for name in layouts: coords = numpy.loadtxt(layouts[name]['filename']) layouts[name]['station_coords'] = coords x = coords[:, 0] y = coords[:, 1] z = coords[:, 2] # TODO(BM) remove stations > xx km r = (x**2 + y**2)**0.5 sort_idx = numpy.argsort(r) r = r[sort_idx] x = x[sort_idx] y = y[sort_idx] z = z[sort_idx] x = x[r <= 5000.0] y = y[r <= 5000.0] z = z[r <= 5000.0] print(name, x.shape) x, y, z = pyuvwsim.convert_enu_to_ecef(x, y, z, lon, lat) uu, vv, ww = generate_baseline_uvw(x, y, z, ra, dec, num_times, mjd_start, dt_s) layouts[name]['uu'] = uu layouts[name]['vv'] = vv layouts[name]['ww'] = ww print('- UV coordinate generation complete.') print('- obs_length = %.2f s (%.2f h)' % (obs_length, obs_length / 3600.0)) print('- num_times =', num_times) # Plotting ================================================================ t0 = time.time() plot_layouts_2(layouts, station_radius_m, join(out_dir, 'layouts')) uv_plot_2(layouts, join(out_dir, 'uv_scatter')) plot_psf_2(layouts, freq_hz, 60.0, 4096, join(out_dir, 'psf')) plot_psf_2(layouts, freq_hz, 30.0, 4096, join(out_dir, 'psf')) plot_psf_2(layouts, freq_hz, 5.0, 4096, join(out_dir, 'psf')) plot_psf_2(layouts, freq_hz, 1.0, 4096, join(out_dir, 'psf')) # plot_uv_hist(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, wave_length, # join(out_dir, 'uv_hist')) # plot_uv_images(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, wave_length, # station_radius_m, join(out_dir, 'uv_images')) # plot_az_rms_2(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, wave_length, # join(out_dir, 'uv_az')) print('- Plotting took %.2f s' % (time.time() - t0))
def main(): # Load station positions t0 = time.time() v4d_file = join('v4d.tm', 'layout_enu_stations.txt') v4o1_file = join('v4o1.tm', 'layout_enu_stations.txt') v4d = numpy.loadtxt(v4d_file) v4o1 = numpy.loadtxt(v4o1_file) station_radius_m = 35.0 / 2.0 num_stations = v4d.shape[0] assert(v4o1.shape[0] == v4d.shape[0]) print('- loading coordinates took %.2f s' % (time.time() - t0)) freq = 100.0e6 wave_length = 299792458.0 / freq lon = radians(116.63128900) lat = radians(-26.69702400) alt = 0.0 ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 snapshot = True if snapshot: mjd_start = mjd_mid obs_length = 0.0 dt_s = 0.0 num_times = 1 else: obs_length = 4.0 * 3600.0 # seconds num_times = int(obs_length / (3 * 60.0)) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - (obs_length / 2.0) / (3600.0 * 24.0) print('- obs_length = %.2f s (%.2f h)' % (obs_length, obs_length / 3600.0)) print('- num_times =', num_times) num_baselines = num_stations * (num_stations - 1) / 2 out_dir = 'uv_%3.1fh' % (obs_length / 3600.0) # UV coordinate generation ================================================ t0 = time.time() x, y, z = convert_enu_to_ecef(v4d[:, 0], v4d[:, 1], v4d[:, 2], lon, lat, alt) uu_v4d, vv_v4d, ww_v4d = \ generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) x, y, z = convert_enu_to_ecef(v4o1[:, 0], v4o1[:, 1], v4o1[:, 2], lon, lat, alt) uu_v4o1, vv_v4o1, ww_v4o1 = \ generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) print('- coordinate generation took %.2f s' % (time.time() - t0)) print('- num vis = %i' % uu_v4d.shape[0]) # Plotting =============================================================== if os.path.exists(out_dir): shutil.rmtree(out_dir) # plot_layouts(v4d, v4o1, station_radius_m, join(out_dir, 'layouts')) # plot_psf(uu_v4d, vv_v4d, ww_v4d, uu_v4o1, vv_v4o1, ww_v4o1, freq, # join(out_dir, 'psf')) # uv_plot(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, join(out_dir, 'uv_scatter')) plot_uv_hist(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, wave_length, join(out_dir, 'uv_hist'))
def main(): # Load station positions t0 = time.time() v4d_file = join('v4d.tm', 'layout_enu_stations.txt') v4o1_file = join('v4o1.tm', 'layout_enu_stations.txt') v4d = numpy.loadtxt(v4d_file) v4o1 = numpy.loadtxt(v4o1_file) station_radius_m = 35.0 / 2.0 num_stations = v4d.shape[0] assert(v4o1.shape[0] == v4d.shape[0]) print('- loading coordinates took %.2f s' % (time.time() - t0)) freq = 120.0e6 wave_length = 299792458.0 / freq lon = radians(116.63128900) lat = radians(-26.69702400) alt = 0.0 ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 snapshot = True if snapshot: mjd_start = mjd_mid obs_length = 0.0 dt_s = 0.0 num_times = 1 else: obs_length = 4.0 * 3600.0 # seconds num_times = int(obs_length / (3 * 60.0)) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - (obs_length / 2.0) / (3600.0 * 24.0) print('- obs_length = %.2f s (%.2f h)' % (obs_length, obs_length / 3600.0)) print('- num_times =', num_times) num_baselines = num_stations * (num_stations - 1) / 2 out_dir = 'uv_%3.1fh' % (obs_length / 3600.0) if os.path.exists(out_dir): shutil.rmtree(out_dir) os.makedirs(out_dir) # UV coordinate generation =============================================== t0 = time.time() x, y, z = convert_enu_to_ecef(v4d[:, 0], v4d[:, 1], v4d[:, 2], lon, lat, alt) uu_v4d, vv_v4d, ww_v4d = \ generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) print('- Coordinate generation took %.2f s' % (time.time() - t0)) print('- Num vis = %i' % uu_v4d.shape[0]) fov = 180.0 # deg im_size = 8192 n = im_size c = n / 2 z = 128 cell_size_lm_arcsec = fov_to_cell_size(fov, im_size) cell_size_uv = grid_cell_size(cell_size_lm_arcsec, im_size) uv_max = ((im_size / 2) - 5) * cell_size_uv uv_r_cut = uv_max * wave_length uv_r = (uu_v4d**2 + vv_v4d**2)**0.5 uv_sort_idx = numpy.argsort(uv_r) uv_r = uv_r[uv_sort_idx] uu_v4d = uu_v4d[uv_sort_idx] vv_v4d = vv_v4d[uv_sort_idx] ww_v4d = ww_v4d[uv_sort_idx] i_uv_max = numpy.argmax(uv_r >= uv_r_cut) uu_v4d = uu_v4d[:i_uv_max] vv_v4d = vv_v4d[:i_uv_max] ww_v4d = ww_v4d[:i_uv_max] print('- No. uv points after radial cut = %i' % uu_v4d.shape[0]) fig = pyplot.figure(figsize=(8, 8)) ax = fig.add_subplot(111, aspect='equal') ax.plot(uu_v4d, vv_v4d, '.', ms=2.0, alpha=0.2) ax.set_xlim(-uv_max * wave_length, uv_max * wave_length) ax.set_ylim(-uv_max * wave_length, uv_max * wave_length) fig.savefig(join(out_dir, 'uv_scatter.png')) pyplot.close(fig) psf_v4d = make_psf(uu_v4d, vv_v4d, ww_v4d, freq, fov, im_size) lm_max = psf_v4d['lm_max'] lm_inc = psf_v4d['lm_inc'] off = lm_inc / 2.0 extent = [-lm_max - off, lm_max - off, -lm_max - off, lm_max - off] plot_image_log(psf_v4d['image'], extent, fov, join(out_dir, 'psf')) print('- Loading beam image.') prefix = 'b_TIME_AVG_CHAN_AVG_CROSS_POWER' beam_amp = pyfits.getdata(join('beams_180.0_120.0MHz', prefix + '_AMP_I_I.fits')) beam_phase = pyfits.getdata(join('beams_180.0_120.0MHz', prefix + '_PHASE_I_I.fits')) beam_amp = numpy.squeeze(beam_amp) beam_phase = numpy.squeeze(beam_phase) beam_amp[numpy.isnan(beam_amp)] = 0.0 beam_phase[numpy.isnan(beam_phase)] = 0.0 beam = beam_amp * numpy.exp(1.0j * beam_phase) # beam /= numpy.sum(beam) print('- beam sum = %f %f' % (numpy.sum(beam.real), numpy.sum(beam_amp))) beam_amp = beam_amp / numpy.nanmax(beam_amp) plot_image_lin(beam_amp, extent, fov, join(out_dir, 'beam_amp')) plot_image_lin(beam_phase, extent, fov, join(out_dir, 'beam_phase')) plot_image_lin(beam_amp[c - z:c + z, c - z:c + z], [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'beam_amp_zoom')) plot_image_lin(numpy.real(beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'beam_re_zoom')) plot_image_lin(numpy.imag(beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'beam_im_zoom')) # Beam uv plane response uv_beam = numpy.fft.fftshift(numpy.fft.ifft2(numpy.fft.fftshift(beam))) plot_image_lin(numpy.real(uv_beam), extent, 0, join(out_dir, 'uv_beam_re')) plot_image_lin(numpy.imag(uv_beam), extent, 0, join(out_dir, 'uv_beam_im')) plot_image_lin(numpy.real(uv_beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_beam_re_zoom')) plot_image_lin(numpy.imag(uv_beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_beam_im_zoom')) print('- Beam x PSF.') beam_psf = beam * psf_v4d['image'] plot_image_log(numpy.real(beam_psf), extent, fov, join(out_dir, 'psf_beam_re')) plot_image_log(numpy.imag(beam_psf), extent, fov, join(out_dir, 'psf_beam_im')) print('- UV image (beam convolved).') uv_psf_beam = numpy.fft.fftshift(numpy.fft.ifft2(numpy.fft.fftshift(beam_psf))) plot_image_lin(numpy.real(uv_psf_beam), [-1, 1, -1, 1], 0, join(out_dir, 'uv_psf_beam_re')) plot_image_lin(numpy.imag(uv_psf_beam), [-1, 1, -1, 1], 0, join(out_dir, 'uv_psf_beam_im')) print('- UV image (PSF only).') uv_psf = numpy.fft.fftshift( numpy.fft.ifft2(numpy.fft.fftshift(psf_v4d['image']))) print('- uv_psf grid sum = %f %f' % (numpy.sum(uv_psf.real), numpy.sum(uv_psf.real))) print('- uv_psf_beam grid sum = %f %f' % (numpy.sum(uv_psf_beam.real), numpy.sum(uv_psf_beam.real))) uv_psf /= numpy.sum(uv_psf) uv_psf_beam /= numpy.sum(uv_psf_beam) uv_psf *= uu_v4d.shape[0] uv_psf_beam *= uu_v4d.shape[0] plot_image_lin(numpy.real(uv_psf), [-1, 1, -1, 1], 0, join(out_dir, 'uv_psf_re')) plot_image_lin(numpy.imag(uv_psf), [-1, 1, -1, 1], 0, join(out_dir, 'uv_psf_im')) plot_image_lin(numpy.real(uv_psf[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_psf_re_zoom')) plot_image_lin(numpy.imag(uv_psf[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_psf_im_zoom')) plot_image_lin(numpy.real(uv_psf_beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_psf_beam_re_zoom')) plot_image_lin(numpy.imag(uv_psf_beam[c - z: c + z, c - z: c + z]), [-z - 0.5, z - 0.5, -z + 0.5, z + 0.5], 0, join(out_dir, 'uv_psf_beam_im_zoom')) # # Grid uv data to compare with FT(psf) wrt normalisation # uv_grid = numpy.zeros((im_size, im_size)) # for i in range(uu_v4d.shape[0]): # gx = round(uu_v4d[i] / cell_size_uv) + (im_size / 2) # gy = round(vv_v4d[i] / cell_size_uv) + (im_size / 2) # uv_grid[gy, gx] += 1 # print('- uv_grid sum = %f' % numpy.sum(uv_grid)) print('- uv_psf sum = %f' % numpy.sum(uv_psf.real)) plot_uv_image(uu_v4d, vv_v4d, cell_size_uv, 250 * cell_size_uv, station_radius_m, join(out_dir, 'uv_image')) print('- Producing Azimuthal averaged plots') # Azimuthal average and plot vs radius _, _, r = image_coords(im_size, lm_inc) x = r.flatten() sort_idx = numpy.argsort(x) x = x[sort_idx] y1 = numpy.real(uv_psf).flatten() y1 = y1[sort_idx] y2 = numpy.real(uv_psf_beam).flatten() y2 = y2[sort_idx] fig = pyplot.figure(figsize=(8, 8)) ax = fig.add_subplot(111) ax.plot(x, y1, 'b.', ms=3.0, alpha=0.1, label='uv') ax.plot(x, y2, 'r.', ms=3.0, alpha=0.1, label='uv convolved with PB') ax.legend() ax.set_xlim(0, 0.1) fig.savefig(join(out_dir, 'az_uv_r.png')) pyplot.close(fig)
# --------------------------------------------------------- filename = '@PROJECT_BINARY_DIR@/test/VLA_A_hor_xyz.txt' lon = 0.0 * (np.pi/180.) lat = 90.0 * (np.pi/180.) alt = 0.0 ra0 = 0.0 * (np.pi/180.) dec0 = 90.0 * (np.pi/180.) ntimes = 10 obs_length = 0.2 # days # --------------------------------------------------------- # Generate coordinates. mjd_start = uvw.datetime_to_mjd(2014, 7, 28, 14, 26, 1.321); (x,y,z) = uvw.load_station_coords(filename) (x,y,z) = uvw.convert_enu_to_ecef(x, y, z, lon, lat, alt) t0 = time.time() for i in range(0, ntimes): mjd = mjd_start (uu_m,vv_m,ww_m) = uvw.evaluate_baseline_uvw(x,y,z, ra0, dec0, mjd) print '- Time taken to evaluate uww coordinates = %.3f ms' % ((time.time()-t0)*1.e3) # Scatter plot of baseline coordinates. plt.ioff() plt_filename = 'test.png' fig = plt.figure(figsize=(6,6)) matplotlib.rcParams.update({'font.size': 10}) scatter_size = 3 fig.add_subplot(1,1,1, aspect='equal') plt.scatter(uu_m, vv_m, c='b', lw = 0, s=scatter_size); plt.scatter(-uu_m, -vv_m, c='r', lw = 0, s=scatter_size);
def simulate(config): telescope = config['sim']['telescope'] obs = config['sim']['observation'] freq_hz = obs['freq_hz'] lon = math.radians(telescope['lon_deg']) lat = math.radians(telescope['lat_deg']) alt = telescope['alt_m'] vis_ra = math.radians(obs['ra_deg']) vis_dec = math.radians(obs['dec_deg']) mjd_start = obs['start_time_mjd'] num_dumps = obs['num_times'] dump_time_s = obs['dump_time_s'] over_sample = obs['over_sample'] dt_s = dump_time_s / over_sample num_times = num_dumps * over_sample telescope_model = telescope['path'] x, y, z = load_station_coords(join(telescope_model, 'layout.txt')) x, y, z = convert_enu_to_ecef(x, y, z, lon, lat, alt) num_antennas = x.shape[0] num_baselines = num_antennas * (num_antennas - 1) / 2 num_vis = num_times * num_baselines sky_model = config['sim']['sky_file'] sky = numpy.loadtxt(sky_model, delimiter=',') sky = sky.reshape((-1, 3)) l, m, n = convert_ra_dec_to_relative_directions(sky[:, 0], sky[:, 1], vis_ra, vis_dec) amp = numpy.zeros(num_vis, dtype='c16') weight = numpy.ones(num_vis, dtype='f8') print('- Simulating data...') print(' - No. antennas :', num_antennas) print(' - No. baselines :', num_baselines) print(' - Obs. length : %.1f s' % (num_dumps * dump_time_s)) print(' - No. times : %i (no. dumps: %i, over-sample: %i)' % (num_times, num_dumps, over_sample)) print(' - No. vis :', num_vis) print(' - No. sources :', sky.shape[0]) num_bytes = num_vis * 7 * 8 mem = virtual_memory() print(' - Mem. required : %.1f / %.1f MB' % (num_bytes / 1024.0**2, mem.total / 1024.0**2)) if num_bytes >= mem.total: raise RuntimeError('Not enough system memory for requested ' 'simulation.') # Generate UVW coordinates. t0 = time.time() uu, vv, ww = generate_baseline_uvw(x, y, z, vis_ra, vis_dec, num_times, num_baselines, mjd_start, dt_s) t_coords = time.time() - t0 # Generate amplitudes. t1 = time.time() wavelength = 299792458.0 / freq_hz for i in range(len(l)): phase = (2.0 * math.pi / wavelength) * \ (uu * l[i] + vv * m[i] + ww * (n[i] - 1.0)) amp += numpy.exp(1.0j * phase) t_amp = time.time() - t1 print(' - Total simulation time = %.2f s (coords: %.2f s, amp: %.2f s)' % (time.time() - t0, t_coords, t_amp)) return {'model': amp, 'uu': uu, 'vv': vv, 'ww': ww, 'weight': weight}
def simulate_2(config): """Simulate with and without corruptions followed by averaging. Simulation to be performed in blocks due to memory constraints. """ telescope = config['sim']['telescope'] obs = config['sim']['observation'] corrupt = config['corrupt'] freq_hz = obs['freq_hz'] wavelength = 299792458.0 / freq_hz lon = math.radians(telescope['lon_deg']) lat = math.radians(telescope['lat_deg']) alt = telescope['alt_m'] ra = math.radians(obs['ra_deg']) dec = math.radians(obs['dec_deg']) mjd_start = obs['start_time_mjd'] num_dumps = obs['num_times'] dump_time_s = obs['dump_time_s'] over_sample = obs['over_sample'] dt_s = dump_time_s / over_sample num_times = num_dumps * over_sample telescope_model = telescope['path'] x, y, z = load_station_coords(join(telescope_model, 'layout.txt')) x, y, z = convert_enu_to_ecef(x, y, z, lon, lat, alt) num_antennas = x.shape[0] num_baselines = num_antennas * (num_antennas - 1) / 2 num_vis = num_dumps * num_baselines sky_model = config['sim']['sky_file'] sky = numpy.loadtxt(sky_model, delimiter=',') sky = sky.reshape((-1, 3)) num_sources = sky.shape[0] source_ra = numpy.radians(sky[:, 0]) source_dec = numpy.radians(sky[:, 1]) l, m, n = convert_ra_dec_to_relative_directions( source_ra, source_dec, ra, dec) tau = corrupt['tau_s'] hurst_amp = corrupt['amplitude']['hurst'] adev_amp = corrupt['amplitude']['allan_dev'] std_t_mid_amp = corrupt['amplitude']['std_t_mid'] hurst_phase = corrupt['phase']['hurst'] adev_phase = corrupt['phase']['allan_dev'] std_t_mid_phase = corrupt['phase']['std_t_mid'] smoothing_length = corrupt['smoothing_length'] print('- Simulating data...') print(' - No. antennas :', num_antennas) print(' - No. baselines :', num_baselines) print(' - Obs. length : %.1f s' % (num_dumps * dump_time_s)) print(' - No. times : %i (no. dumps: %i, over-sample: %i)' % (num_times, num_dumps, over_sample)) print(' - No. vis :', num_vis) print(' - No. sources :', num_sources) print(' - Corruptions:') print(' - Hurst amp %.1f, phase %.1f' % (hurst_amp, hurst_phase)) print(' - A. dev amp %.1e, phase %.1e' % (adev_amp, adev_phase)) num_bytes = num_vis * 8 * 8 + (num_antennas * num_times) * 16 mem = virtual_memory() print(' - Mem. required : %.1f / %.1f MB' % (num_bytes / 1024.0**2, mem.total / 1024.0**2)) if num_bytes >= mem.total: raise RuntimeError('Not enough system memory for requested ' 'simulation.') # Generate corruptions gains = numpy.empty((num_antennas, num_times), dtype='c16') t0 = time.time() for i in range(num_antennas): gains[i, :] = eval_complex_gains(num_times, dt_s, hurst_amp, adev_amp, std_t_mid_amp, hurst_phase, adev_phase, std_t_mid_phase, smoothing_length, tau) conj_gains = numpy.conj(gains) print(' - Gains generated in %.1f s' % (time.time() - t0)) # TODO-BM plot the gains ... # Simulation phase0 = 2.0 * math.pi / wavelength model = numpy.empty(num_vis, dtype='c16') data = numpy.empty(num_vis, dtype='c16') weight = numpy.ones(num_vis, dtype='f8') block_model = numpy.empty((over_sample, num_baselines), dtype='c16') block_data = numpy.empty((over_sample, num_baselines), dtype='c16') t1 = time.time() # Loop over correlator dumps for i in range(num_dumps): block_model.fill(0.0 + 0.0j) block_data.fill(0.0 + 0.0j) # Loop over times in a dump. for t in range(over_sample): delta_t = (i * dump_time_s) + (t * dt_s) + (dt_s / 2.0) mjd = mjd_start + (delta_t / 86400.0) uu_, vv_, ww_ = evaluate_baseline_uvw(x, y, z, ra, dec, mjd) for s in range(num_sources): phase = phase0 * (uu_ * l[s] + vv_ * m[s] + ww_ * (n[s] - 1.0)) block_model[t, :] += numpy.exp(1.0j * phase) ig = i * over_sample + t block_data[t, :] = apply_gains(block_model[t, :], gains[:, ig]) # data_ = apply_gains(block_model[t, :], gains[:, ig]) # idx = 0 # for p in range(num_antennas): # for q in range(p + 1, num_antennas): # gp = gains[p, ig] # gq = conj_gains[q, ig] # block_data[t, idx] = gp * block_model[t, idx] * gq # idx += 1 # if i < 3: # print('t[%02i]' % t) # print(' C:', data_[0]) # print(' P:', block_data[t, 0]) # print(' D:', numpy.max(numpy.abs(data_[:] - block_data[t, :]))) # assert numpy.max(numpy.abs(data_[:] - block_data[t, :])) == 0.0 # Average the block to get visibility data amplitudes for the dump. b0 = i * num_baselines b1 = b0 + num_baselines model[b0:b1] = numpy.mean(block_model, axis=0) data[b0:b1] = numpy.mean(block_data, axis=0) uu, vv, ww = generate_baseline_uvw(x, y, z, ra, dec, num_dumps, num_baselines, mjd_start, dump_time_s) print(' - Visibilities simulated in %.2f s' % (time.time() - t1)) return {'model': model, 'data': data, 'uu': uu, 'vv': vv, 'ww': ww, 'weight': weight, 'num_baselines': num_baselines, 'num_times': num_dumps, 'num_antennas': num_antennas}
def main(): """ 1. Generate a large-ish core of stations using random generator. a. overlap some stations in the core to have a very dense station region 2. After core area start using arms but generate some randomness in the arms by placing antennas randomly near the outer stations keeping them along the spiral 3. Remove radius redundancy in the spiral arms """ # ========================================================================= # ====== Core seed = 1 num_tries = 10 num_core_stations = (1 + 5 + 11 + 17) * 6 + (3 * 6) core_radius_m = 480.0 inner_core_radius_m = 280.0 station_radius_m = 35.0 / 2.0 sll = -28 # ====== Core arms num_arms = 3 core_arm_count = 4 stations_per_arm_cluster = 6 arm_cluster_radius = 75.0 # a = 300.0 # b = 0.513 a = 300.0 b = 0.513 delta_theta = math.radians(37.0) arm_offsets = numpy.radians([35.0, 155.0, 270.0]) num_core_arm_stations = num_arms * core_arm_count * stations_per_arm_cluster # ====== Outer arms outer_arm_count = 12 stations_per_outer_cluster = 6 num_clusters_outer = outer_arm_count * num_arms v4a_ss_enu_file = 'v7ska1lowN1v2rev3R.enu.94x4.fixed.txt' outer_arm_cluster_radius = 80.0 # ===== uvw coordinate generation. lon = radians(116.63128900) lat = radians(-26.69702400) alt = 0.0 ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 obs_length = 0.0 mjd_start = mjd_mid dt_s = 0.0 num_times = 1 obs_length = 2.0 * 3600.0 # seconds num_times = int(obs_length / (3.0 * 60.0)) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - ((obs_length / 2.0) / 3600.0 * 24.0) print('num times = %i' % num_times) out_dir = 'v5c-2h' # ========================================================================= if not os.path.isdir(out_dir): os.makedirs(out_dir) # Generate core stations x_core, y_core, weights, r_weights = \ generate_random_core(num_core_stations, core_radius_m, inner_core_radius_m, sll, station_radius_m, num_tries, seed) # Core arms x_arm, y_arm, cx_arm, cy_arm = \ generate_core_arms(num_arms, core_arm_count, stations_per_arm_cluster, arm_cluster_radius, station_radius_m, a, b, delta_theta, arm_offsets, num_tries) # Outer stations. x_arm_outer, y_arm_outer, cx_outer, cy_outer = \ generate_outer_arms(v4a_ss_enu_file, num_clusters_outer, stations_per_outer_cluster, outer_arm_cluster_radius, station_radius_m, num_tries) # Plotting plot_layout(x_core, y_core, x_arm, y_arm, x_arm_outer, y_arm_outer, cx_arm, cy_arm, cx_outer, cy_outer, station_radius_m, inner_core_radius_m, core_radius_m, arm_cluster_radius, outer_arm_cluster_radius, out_dir) plot_core_thinning_profile(r_weights, weights, core_radius_m, inner_core_radius_m, out_dir) if uvwsim_found: x = numpy.hstack((x_core, x_arm, x_arm_outer)) y = numpy.hstack((y_core, y_arm, y_arm_outer)) print('total stations = %i' % x.shape[0]) num_stations = x.shape[0] z = numpy.zeros_like(x) num_baselines = num_stations * (num_stations - 1) / 2 x, y, z = convert_enu_to_ecef(x, y, z, lon, lat, alt) uu, vv, ww = generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) plot_hist(uu, vv, join(out_dir, 'uv_hist_%.2fh.png' % (obs_length/3600.0)), 'v5c %.2f h' % (obs_length/3600.0)) plot_uv_dist(uu, vv, station_radius_m, join(out_dir, 'uv_%.2fh' % (obs_length/3600.0))) # TODO-BM see ALMA memo for plots? # TODO-BM Plot of azimuthal variation # TODO-BM movie of uv coverage histogram improvement with time? # TODO-BM convolve uv response with station beam?! print('making image...') imager = Imager('single') fov = 1.0 im_size = 2048 freq = 150.0e6 wavelength = 299792458.0 / freq uu /= wavelength vv /= wavelength ww /= wavelength amp = numpy.ones(uu.shape, dtype='c16') weight = numpy.ones(uu.shape, dtype='f8') image = imager.make_image(uu, vv, ww, amp, weight, fov, im_size) fig = pyplot.figure(figsize=(8, 8)) ax = fig.add_subplot(111, aspect='equal') ax.imshow(image, interpolation='nearest') pyplot.show() cell = math.degrees(imager.fov_to_cellsize(math.radians(fov), im_size)) save_fits_image_2(join(out_dir, 'psf.fits'), image, cell, math.degrees(ra), math.degrees(dec), freq)
def main(): print("*" * 80) print("*" * 80) print("THIS SCRIPT IS DEPRECATED IN FAVOUR OF: generate_uv_coverage_2.py") print("*" * 80) print("*" * 80) return # Load station positions t0 = time.time() v4d_file = join("v4d.tm", "layout_enu_stations.txt") v4o1_file = join("v4o1.tm", "layout_enu_stations.txt") v4d = numpy.loadtxt(v4d_file) v4o1 = numpy.loadtxt(v4o1_file) station_radius_m = 35.0 / 2.0 num_stations = v4d.shape[0] assert v4o1.shape[0] == v4d.shape[0] print("- loading coordinates took %.2f s" % (time.time() - t0)) freq = 100.0e6 wave_length = 299792458.0 / freq lon = radians(116.63128900) lat = radians(-26.69702400) alt = 0.0 ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 snapshot = True if snapshot: mjd_start = mjd_mid obs_length = 0.0 dt_s = 0.0 num_times = 1 else: obs_length = 4.0 * 3600.0 # seconds num_times = int(obs_length / (3 * 60.0)) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - (obs_length / 2.0) / (3600.0 * 24.0) print("- obs_length = %.2f s (%.2f h)" % (obs_length, obs_length / 3600.0)) print("- num_times =", num_times) num_baselines = num_stations * (num_stations - 1) / 2 out_dir = "uv_%3.1fh" % (obs_length / 3600.0) if not os.path.isdir(out_dir): os.makedirs(out_dir) # plot_layouts(v4d, v4o1, station_radius_m, out_dir) # t0 = time.time() x, y, z = convert_enu_to_ecef(v4d[:, 0], v4d[:, 1], v4d[:, 2], lon, lat, alt) uu_v4d, vv_v4d, ww_v4d = generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) x, y, z = convert_enu_to_ecef(v4o1[:, 0], v4o1[:, 1], v4o1[:, 2], lon, lat, alt) uu_v4o1, vv_v4o1, ww_v4o1 = generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) print("- coordinate generation took %.2f s" % (time.time() - t0)) print("- num vis = %i" % uu_v4d.shape[0]) # t0 = time.time() # uv_plot(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, out_dir) # print('- uv scatter plot took %.2f s' % (time.time() - t0)) # t0 = time.time() # v4d_uv_dist = (uu_v4d**2 + vv_v4d**2)**0.5 # v4d_uv_dist.sort() # v4o1_uv_dist = (uu_v4o1**2 + vv_v4o1**2)**0.5 # v4o1_uv_dist.sort() # hist_plot_1(v4d_uv_dist, v4o1_uv_dist, wave_length, 300.0, out_dir) # hist_plot_1(v4d_uv_dist, v4o1_uv_dist, wave_length * 5.0, 1500.0, out_dir) # hist_plot_1(v4d_uv_dist, v4o1_uv_dist, wave_length, 1500.0, out_dir) # hist_plot_1(v4d_uv_dist, v4o1_uv_dist, wave_length * 10.0, 3000.0, out_dir) # print('- histograms took %.2f s' % (time.time() - t0)) # # hist_plot_2(v4d_uv_dist, v4o1_uv_dist, wave_length, out_dir) # hist_plot_3(v4d_uv_dist, v4o1_uv_dist, wave_length, out_dir) # plot_uv_images(uu_v4d, vv_v4d, uu_v4o1, vv_v4o1, wave_length, station_radius_m, out_dir) make_psf_images(uu_v4d, vv_v4d, ww_v4d, uu_v4o1, vv_v4o1, ww_v4o1, ra, dec, freq, out_dir)
def main(): # ========================================================================== # Telescope element radii st_radius = 35.0 / 2.0 # Station-radius ss_radius = st_radius * 3.0 # Super-station radius # Core ring super-stations num_rings = 4 ring_counts = [1, 5, 11, 17] ring_radii = [0.0, 100.0, 190.0, 290.0] # metres num_super_stations_rings = numpy.array(ring_counts).sum() ring_start_angle = -360.0 * random(num_rings) + 360.0 ss_ring_petal_angle = -360.0 * random(num_super_stations_rings) + 360.0 # Core arms num_arms = 3 core_arm_count = 5 # Number of super-stations per core arm a = 300.0 b = 0.513 delta_theta = 37.0 arm_offsets = [35.0, 155.0, 275.0] num_super_stations_arms = num_arms * core_arm_count ss_arm_petal_angle = -360.0 * random(num_super_stations_arms) + 360.0 # Outer arms (same outer 3 * 12 = 36 stations as v4a) outer_arm_count = 12 # Number of super-stations per outer arm num_super_stations_outer = num_arms * outer_arm_count v4a_ss_enu_file = 'v7ska1lowN1v2rev3R.enu.94x4.fixed.txt' ss_petal_angle_outer = -360.0 * random(num_super_stations_outer) + 360.0 # Stations num_stations_per_ss = 6 out_dir = 'v4d_layout' if not os.path.isdir(out_dir): os.makedirs(out_dir) # ========================================================================== # == Super-stations # Generate core ring super-stations v4d_ss_x_rings = numpy.zeros(num_super_stations_rings) v4d_ss_y_rings = numpy.zeros(num_super_stations_rings) idx = 0 for i, hist in enumerate(ring_counts): angles = numpy.arange(hist) * (360.0 / hist) angles += ring_start_angle[i] x = ring_radii[i] * numpy.cos(numpy.radians(angles)) y = ring_radii[i] * numpy.sin(numpy.radians(angles)) v4d_ss_x_rings[idx:idx+hist] = x v4d_ss_y_rings[idx:idx+hist] = y idx += hist # Generate core spiral arm super-stations v4d_ss_x_arms = numpy.zeros(num_super_stations_arms) v4d_ss_y_arms = numpy.zeros(num_super_stations_arms) for i in range(num_arms): t = numpy.arange(1, core_arm_count + 1) * delta_theta t = numpy.radians(t) x = a * numpy.exp(b * t) * numpy.cos(t + numpy.radians(arm_offsets[i])) y = a * numpy.exp(b * t) * numpy.sin(t + numpy.radians(arm_offsets[i])) i0 = i * core_arm_count i1 = i0 + core_arm_count v4d_ss_x_arms[i0:i1] = x v4d_ss_y_arms[i0:i1] = y # Load super-station outer spiral arms from the v4a config v4a_ss_enu = numpy.loadtxt(v4a_ss_enu_file) v4a_ss_enu = v4a_ss_enu[:, 1:] v4a_ss_r = (v4a_ss_enu[:, 0]**2 + v4a_ss_enu[:, 1]**2)**0.5 sort_idx = numpy.argsort(v4a_ss_r) v4a_ss_enu = v4a_ss_enu[sort_idx[::-1], :] v4d_ss_x_outer = v4a_ss_enu[:num_super_stations_outer, 0] v4d_ss_y_outer = v4a_ss_enu[:num_super_stations_outer, 1] # == Stations # Generate core ring stations v4d_st_x_rings = numpy.zeros((num_super_stations_rings, num_stations_per_ss)) v4d_st_y_rings = numpy.zeros_like(v4d_st_x_rings) for i in range(num_super_stations_rings): angles = 360.0 / (num_stations_per_ss - 1) * \ numpy.arange(num_stations_per_ss - 1) x = (st_radius * 2.0) * numpy.cos(numpy.radians(angles)) y = (st_radius * 2.0) * numpy.sin(numpy.radians(angles)) x, y = rotate_coords(x, y, ss_ring_petal_angle[i]) v4d_st_x_rings[i, 1:] = x v4d_st_y_rings[i, 1:] = y v4d_st_x_rings[i, :] += v4d_ss_x_rings[i] v4d_st_y_rings[i, :] += v4d_ss_y_rings[i] v4d_st_x_rings = v4d_st_x_rings.flatten() v4d_st_y_rings = v4d_st_y_rings.flatten() # Generate core spiral arm stations v4d_st_x_arms = numpy.zeros((num_super_stations_arms, num_stations_per_ss)) v4d_st_y_arms = numpy.zeros_like(v4d_st_x_arms) for i in range(num_super_stations_arms): angles = 360.0 / (num_stations_per_ss - 1) * \ numpy.arange(num_stations_per_ss - 1) x = (st_radius * 2.0) * numpy.cos(numpy.radians(angles)) y = (st_radius * 2.0) * numpy.sin(numpy.radians(angles)) x, y = rotate_coords(x, y, ss_arm_petal_angle[i]) v4d_st_x_arms[i, 1:] = x v4d_st_y_arms[i, 1:] = y v4d_st_x_arms[i, :] += v4d_ss_x_arms[i] v4d_st_y_arms[i, :] += v4d_ss_y_arms[i] v4d_st_x_arms = v4d_st_x_arms.flatten() v4d_st_y_arms = v4d_st_y_arms.flatten() # Generate outer arm stations v4d_st_x_outer = numpy.zeros((num_super_stations_outer, num_stations_per_ss)) v4d_st_y_outer = numpy.zeros((num_super_stations_outer, num_stations_per_ss)) for i in range(num_super_stations_outer): angles = 360.0 / (num_stations_per_ss - 1) * \ numpy.arange(num_stations_per_ss - 1) x = (st_radius * 2.0) * numpy.cos(numpy.radians(angles)) y = (st_radius * 2.0) * numpy.sin(numpy.radians(angles)) x, y = rotate_coords(x, y, ss_petal_angle_outer[i]) v4d_st_x_outer[i, 1:] = x v4d_st_y_outer[i, 1:] = y v4d_st_x_outer[i, :] += v4d_ss_x_outer[i] v4d_st_y_outer[i, :] += v4d_ss_y_outer[i] v4d_st_x_outer = v4d_st_x_outer.flatten() v4d_st_y_outer = v4d_st_y_outer.flatten() # Concatenate coords. v4d_ss_x = numpy.hstack((v4d_ss_x_rings, v4d_ss_x_arms, v4d_ss_x_outer)) v4d_ss_y = numpy.hstack((v4d_ss_y_rings, v4d_ss_y_arms, v4d_ss_y_outer)) v4d_st_x = numpy.hstack((v4d_st_x_rings, v4d_st_x_arms, v4d_st_x_outer)) v4d_st_y = numpy.hstack((v4d_st_y_rings, v4d_st_y_arms, v4d_st_y_outer)) # === Generate layouts ============================== num_stations = v4d_st_x.shape[0] v4d_st_enu = numpy.zeros((num_stations, 3)) v4d_st_enu[:, 0] = v4d_st_x v4d_st_enu[:, 1] = v4d_st_y numpy.savetxt(join(out_dir, 'v4d_stations_enu.txt'), v4d_st_enu, fmt='% -16.12f % -16.12f % -16.12f') num_super_stations = v4d_ss_x.shape[0] v4d_ss_enu = numpy.zeros((num_super_stations, 3)) v4d_ss_enu[:, 0] = v4d_ss_x v4d_ss_enu[:, 1] = v4d_ss_y numpy.savetxt(join(out_dir, 'v4d_super_stations_enu.txt'), v4d_ss_enu, fmt='% -16.12f % -16.12f % -16.12f') # ==== Plotting =========================================================== fig = pyplot.figure(figsize=(8, 8)) ax = fig.add_subplot(111, aspect='equal') for i in range(num_super_stations_rings): circle = pyplot.Circle((v4d_ss_x_rings[i], v4d_ss_y_rings[i]), ss_radius, color='b', fill=True, alpha=0.5, linewidth=0.0) ax.add_artist(circle) arm_colors = ['y', 'g', 'r'] for i in range(num_super_stations_arms): q = int(i / core_arm_count) circle = pyplot.Circle((v4d_ss_x_arms[i], v4d_ss_y_arms[i]), ss_radius, color=arm_colors[q], fill=True, alpha=0.5, linewidth=0.0) ax.add_artist(circle) for q in range(num_arms): i0 = q * outer_arm_count i1 = i0 + outer_arm_count for i in range(i0, i1): circle = pyplot.Circle((v4d_ss_x_outer[i], v4d_ss_y_outer[i]), ss_radius, color='c', fill=True, alpha=0.5) ax.add_artist(circle) # Plot station positions for i in range(v4d_st_x.shape[0]): circle = pyplot.Circle((v4d_st_x[i], v4d_st_y[i]), st_radius, color='k', linewidth=1.0, fill=True, alpha=0.2) ax.add_artist(circle) # circle = pyplot.Circle((0.0, 0.0), 1700.0, color='r', linestyle='--', # linewidth=1.0, fill=False, alpha=0.5) # ax.add_artist(circle) ax.grid(which='both') ax.grid(which='minor', alpha=0.5) ax.grid(which='major', alpha=1.0) ax.set_ylabel('North [m]') ax.set_xlabel('East [m]') ax.set_xlim(-1500, 1500) ax.set_ylim(-1500, 1500) pyplot.savefig(join(out_dir, 'v4d_station_layout_zoom_1.5km.png')) ax.set_xlim(-3000, 3000) ax.set_ylim(-3000, 3000) pyplot.savefig(join(out_dir, 'v4d_station_layout_zoom_3.0km.png')) ax.set_xlim(-5000, 5000) ax.set_ylim(-5000, 5000) pyplot.savefig(join(out_dir, 'v4d_station_layout_zoom_5.0km.png')) ax.set_xlim(-50000, 50000) ax.set_ylim(-50000, 50000) pyplot.savefig(join(out_dir, 'v4d_station_layout_50.0km.png')) pyplot.close(fig) if uvwsim_found: # TODO-BM make this a function in layout_utils.py print('generating uv coords...') x = v4d_st_x y = v4d_st_y num_stations = x.shape[0] z = numpy.zeros_like(x) lon = radians(116.63128900) lat = radians(-26.69702400) alt = 0.0 ra = radians(68.698903779331502) dec = radians(-26.568851215532160) mjd_mid = 57443.4375000000 obs_length = 4.0 * 3600.0 # seconds num_times = int(obs_length / (3 * 60.0)) # print('num_times =', num_times) dt_s = obs_length / float(num_times) mjd_start = mjd_mid - (obs_length / 2.0) / (3600.0 * 24.0) mjd_start = mjd_mid obs_length = 0.0 dt_s = 0.0 num_times = 1 num_baselines = num_stations * (num_stations - 1) / 2 x, y, z = convert_enu_to_ecef(x, y, z, lon, lat, alt) uu, vv, ww = generate_baseline_uvw(x, y, z, ra, dec, num_times, num_baselines, mjd_start, dt_s) layout_utils.plot_hist(uu, vv, join(out_dir, 'v4d_hist.png'), 'v4d snapshot-uv') layout_utils.plot_uv_dist(uu, vv, st_radius, join(out_dir, 'v4d_snapshot_uv_zenith')) layout_utils.plot_uv_grid_image(uu, vv, 5.0, join(out_dir, 'uv_image'))
# --------------------------------------------------------- filename = '@PROJECT_BINARY_DIR@/test/VLA_A_hor_xyz.txt' lon = 0.0 * (np.pi / 180.) lat = 90.0 * (np.pi / 180.) alt = 0.0 ra0 = 0.0 * (np.pi / 180.) dec0 = 90.0 * (np.pi / 180.) ntimes = 10 obs_length = 0.2 # days # --------------------------------------------------------- # Generate coordinates. mjd_start = uvw.datetime_to_mjd(2014, 7, 28, 14, 26, 1.321) (x, y, z) = uvw.load_station_coords(filename) (x, y, z) = uvw.convert_enu_to_ecef(x, y, z, lon, lat, alt) t0 = time.time() for i in range(0, ntimes): mjd = mjd_start (uu_m, vv_m, ww_m) = uvw.evaluate_baseline_uvw(x, y, z, ra0, dec0, mjd) print '- Time taken to evaluate uww coordinates = %.3f ms' % ( (time.time() - t0) * 1.e3) # Scatter plot of baseline coordinates. plt.ioff() plt_filename = 'test.png' fig = plt.figure(figsize=(6, 6)) matplotlib.rcParams.update({'font.size': 10}) scatter_size = 3 fig.add_subplot(1, 1, 1, aspect='equal') plt.scatter(uu_m, vv_m, c='b', lw=0, s=scatter_size)