示例#1
0
文件: utils.py 项目: whigg/sharad
def get_pik(orbit):
    """Extract surface echo values (convert in linear amplitude)

    Arguments
    ---------
    orbit : string
        orbit number

    Keywords
    --------
    amplitude : bool
        output as linear amplitude
    abs_calib : float
        calibration value
    """
    pik = raw.read_pik(orbit)
    rpb = raw.read_rpb(orbit)

    z = np.round(pik.delay_pixel) - 1
    x = pik.frame - 1
    x = x.values.tolist()

    echo = np.zeros(np.size(x))
    for i, val in enumerate(x):
        try:
            echo[i] = rpb[z[i] - 2:z[i] + 2, val].max()
        except:
            echo[i] = np.nan

    out = np.empty(rpb.shape[1])
    out[x] = echo

    return out
示例#2
0
文件: utils.py 项目: cgrima/sharad
def get_pik(orbit):
    """Extract surface echo values (convert in linear amplitude)

    Arguments
    ---------
    orbit : string
        orbit number

    Keywords
    --------
    amplitude : bool
        output as linear amplitude
    abs_calib : float
        calibration value
    """
    pik = raw.read_pik(orbit)
    rpb = raw.read_rpb(orbit)

    z = np.round(pik.delay_pixel)-1
    x = pik.frame-1
    x = x.values.tolist()

    echo = np.zeros(np.size(x))
    for i, val in enumerate(x):
        try:
            echo[i] = rpb[z[i]-2:z[i]+2, val].max()
        except:
            echo[i] = np.nan


    out = np.empty(rpb.shape[1])
    out[x] = echo

    return out
示例#3
0
文件: utils.py 项目: cgrima/sharad
def get_aux(orbit):
    """Interpolate auxilliary values to echo sampling

    Arguments
    ---------
    orbit : string
        orbit number
    """
    aux = raw.read_aux(orbit)
    rpb = raw.read_rpb(orbit)
    xnew   = np.arange(rpb.shape[1])
    x = np.linspace(0, rpb.shape[1]-1, aux.UTC.size)

    tck = splrep(x, aux.lon, s=0)
    lon = splev(xnew, tck, der=0)

    tck = splrep(x, aux.lat, s=0)
    lat = splev(xnew, tck, der=0)

    tck = splrep(x, aux.radius, s=0)
    radius = splev(xnew, tck, der=0)

    tck = splrep(x, aux.vtan, s=0)
    vtan = splev(xnew, tck, der=0)

    tck = splrep(x, aux.vrad, s=0)
    vrad = splev(xnew, tck, der=0)

    tck = splrep(x, aux.SZA, s=0)
    sza = splev(xnew, tck, der=0)

    tck = splrep(x, aux.pitch, s=0)
    pitch = splev(xnew, tck, der=0)

    tck = splrep(x, aux.yaw, s=0)
    yaw = splev(xnew, tck, der=0)

    tck = splrep(x, aux.roll, s=0)
    roll = splev(xnew, tck, der=0)

    tck = splrep(x, aux.Mag_field, s=0)
    mag = splev(xnew, tck, der=0)

    tck = splrep(x, aux.HGAout, s=0)
    HGAout = splev(xnew, tck, der=0)

    tck = splrep(x, aux.HGAin, s=0)
    HGAin = splev(xnew, tck, der=0)

    tck = splrep(x, aux.Sun_dist, s=0)
    sun_dist = splev(xnew, tck, der=0)

    rng = radius*1e3 - ellipsoid.lonlat2rad(lon, lat, mars.radius['val'])

    out = {'lat':lat, 'lon':lon, 'radius':radius, 'vtan':vtan, 'vrad':vrad,
           'sza':sza, 'pitch':pitch, 'yaw':yaw, 'roll':roll, 'mag':mag,
           'HGAout':HGAout, 'HGAin':HGAin, 'sun_dist':sun_dist, 'rng':rng}
    return pd.DataFrame(out)
示例#4
0
文件: utils.py 项目: whigg/sharad
def get_aux(orbit):
    """Interpolate auxilliary values to echo sampling

    Arguments
    ---------
    orbit : string
        orbit number
    """
    aux = raw.read_aux(orbit)
    rpb = raw.read_rpb(orbit)
    xnew = np.arange(rpb.shape[1])
    x = np.linspace(0, rpb.shape[1] - 1, aux.UTC.size)

    tck = splrep(x, aux.lon, s=0)
    lon = splev(xnew, tck, der=0)

    tck = splrep(x, aux.lat, s=0)
    lat = splev(xnew, tck, der=0)

    tck = splrep(x, aux.radius, s=0)
    radius = splev(xnew, tck, der=0)

    tck = splrep(x, aux.vtan, s=0)
    vtan = splev(xnew, tck, der=0)

    tck = splrep(x, aux.vrad, s=0)
    vrad = splev(xnew, tck, der=0)

    tck = splrep(x, aux.SZA, s=0)
    sza = splev(xnew, tck, der=0)

    tck = splrep(x, aux.pitch, s=0)
    pitch = splev(xnew, tck, der=0)

    tck = splrep(x, aux.yaw, s=0)
    yaw = splev(xnew, tck, der=0)

    tck = splrep(x, aux.roll, s=0)
    roll = splev(xnew, tck, der=0)

    tck = splrep(x, aux.Mag_field, s=0)
    mag = splev(xnew, tck, der=0)

    tck = splrep(x, aux.HGAout, s=0)
    HGAout = splev(xnew, tck, der=0)

    tck = splrep(x, aux.HGAin, s=0)
    HGAin = splev(xnew, tck, der=0)

    tck = splrep(x, aux.Sun_dist, s=0)
    sun_dist = splev(xnew, tck, der=0)

    rng = radius * 1e3 - ellipsoid.lonlat2rad(lon, lat, mars.radius['val'])

    out = {
        'lat': lat,
        'lon': lon,
        'radius': radius,
        'vtan': vtan,
        'vrad': vrad,
        'sza': sza,
        'pitch': pitch,
        'yaw': yaw,
        'roll': roll,
        'mag': mag,
        'HGAout': HGAout,
        'HGAin': HGAin,
        'sun_dist': sun_dist,
        'rng': rng
    }
    return pd.DataFrame(out)