Example #1
0
File: obs.py Project: cilori/SWAMpy
def sam_obs():
    if __name__ == 'sen2coral2.obs':
        print(
            os.path.isfile(
                'bioopti_data\\..\\sambuca\\reference\\wl_alos_data\\inputs\\WL_ALOS_R_0_sub120.img'
            ))

        base_path = 'bioopti_data\\'

        observed_rrs_base_path = base_path + '..\\sambuca\\reference\\wl_alos_data\\inputs\\'
        observed_rrs_raster_path = join(observed_rrs_base_path,
                                        'WL_ALOS_R_0_sub120.img')

        sensor_filter_path = join(base_path, 'sensor_filters')
        sensor_filter_name = 'ALOS'

        substrate_path = join(base_path, 'Substrates')
        substrate1_name = 'moreton_bay_speclib:white Sand'
        substrate2_name = 'moreton_bay_speclib:brown Mud'
        substrate3_name = 'moreton_bay_speclib:Syringodium isoetifolium'
        substrate4_name = 'moreton_bay_speclib:brown algae'
        substrate5_name = 'moreton_bay_speclib:green algae'
        #substrate_names= ( substrate1_name, substrate2_name)
        #substrate_names= ( substrate1_name, substrate2_name, substrate3_name)
        #substrate_names= ( substrate1_name, substrate2_name, substrate3_name, substrate4_name)
        substrate_names = (substrate1_name, substrate2_name, substrate3_name,
                           substrate4_name, substrate5_name)

        aphy_star_path = join(base_path, 'SIOP/WL08_aphy_1nm.hdr')
        aphy_star_name = 'wl08_aphy_1nm:WL08_aphy_star_mean_correct.csv:C2'

        awater_path = join(base_path, 'SIOP/aw_350_900_lw2002_1nm.csv')
        awater_name = 'aw_350_900_lw2002_1nm:a_water'

        nedr_path = join(observed_rrs_base_path, 'WL_ALOS_NEDR_0_4bands.hdr')

        sensor_filter_path = join(base_path, 'sensor_filters')
        sensor_filter_name = 'ALOS'
        observed_rrs_width = 0
        observed_rrs_height = 0
        observed_rrs = None

        with rasterio.drivers():
            with rasterio.open(observed_rrs_raster_path) as src:
                print('Observed rrs file: ', observed_rrs_raster_path)
                print('Width, height: ', src.width, src.height)
                print('crs: ', src.crs)
                print('affine: ', src.affine)
                print('num bands: ', src.count)
                print('band indicies: ', src.indexes)

                observed_rrs_width = src.width
                observed_rrs_height = src.height
                observed_rrs = src.read()

        all_substrates = sbc.load_all_spectral_libraries(substrate_path)
        substrates = []
        for substrate_name in substrate_names:
            substrates.append(all_substrates[substrate_name])
        # load all filters from the given directory
        sensor_filters = sbc.load_sensor_filters(sensor_filter_path)

        # We don't need to do this, but it lets us see the name of all loaded filters
        sensor_filters.keys()

        # retrieve the specified filter
        sensor_filter = sensor_filters[sensor_filter_name]

        #Plot the sensor filter:
        #plot_items.clear()  #Python 3.3 and later only
        aphy_star = sbc.load_spectral_library(aphy_star_path)[aphy_star_name]
        awater = sbc.load_spectral_library(awater_path)[awater_name]
        nedr = sbc.load_spectral_library(
            nedr_path, validate=False)['wl_alos_nedr_0_4bands:33']
        nedr

        wavelengths = sbc.spectra_find_common_wavelengths(
            awater, aphy_star, *substrates)
        print('Common wavelength range: {0} - {1}'.format(
            min(wavelengths), max(wavelengths)))

        #Use the common wavelengths to mask the inputs:
        awater = sbc.spectra_apply_wavelength_mask(awater, wavelengths)
        aphy_star = sbc.spectra_apply_wavelength_mask(aphy_star, wavelengths)
        for i, substrate in enumerate(substrates):
            substrates[i] = sbc.spectra_apply_wavelength_mask(
                substrate, wavelengths)

        print('awater: min: {0}  max: {1}'.format(min(awater[0]),
                                                  max(awater[0])))
        print('aphy_star: min: {0}  max: {1}'.format(min(aphy_star[0]),
                                                     max(aphy_star[0])))
        for substrate_name, substrate in zip(substrate_names, substrates):
            print('{0}: min: {1}  max: {2}'.format(substrate_name,
                                                   min(substrate[0]),
                                                   max(substrate[0])))
        """Truncate the sensor filter to match the common wavelength range
        It remains to be seen whether this is the best approach, but it works for this demo. An alternative approach would be to truncate the entire band for any band that falls outside the common wavelength range.
        If this approach, or something based on it, is valid, then this should be moved into a sambuca_core function with appropriate unit tests."""

        filter_mask = (sensor_filter[0] >= wavelengths.min()) & (
            sensor_filter[0] <= wavelengths.max())
        sensor_filter = sensor_filter[0][filter_mask], sensor_filter[
            1][:, filter_mask]
        xstart = 0
        xend = 10
        xspan = xend - xstart
        ystart = 0
        yend = 120
        print('CIAO ', xstart)
        num_pixels = xspan * (yend - ystart)
        assert xend <= observed_rrs_width
        assert yend <= observed_rrs_height
        fixed_parameters = sb.create_fixed_parameter_set(
            wavelengths=wavelengths,
            a_water=awater,
            a_ph_star=aphy_star,
            substrates=substrates,
        )
        result_recorder = sb.ArrayResultWriter(observed_rrs_width,
                                               observed_rrs_height,
                                               sensor_filter, nedr,
                                               fixed_parameters)
        objective = sb.SciPyObjective(sensor_filter,
                                      fixed_parameters,
                                      error_function=sb.distance_f,
                                      nedr=nedr)

        return wavelengths, observed_rrs, observed_rrs_width, observed_rrs_height, awater, aphy_star, substrates, nedr, sensor_filter, xstart, xend, ystart, yend, num_pixels, fixed_parameters, result_recorder, objective
Example #2
0
def input_prepare(siop, envmeta, image_info, error_name):

    a_water = siop['a_water']
    a_ph_star = siop['a_ph_star']
    substrates = siop['substrates']
    substrate_names = siop['substrate_names']
    sensor_filter = image_info['sensor_filter']
    observed_rrs_width = image_info['observed_rrs_width']
    observed_rrs_height = image_info['observed_rrs_height']
    nedr = image_info['nedr']

    wavelengths = sbc.spectra_find_common_wavelengths(a_water, a_ph_star,
                                                      *substrates)
    #TODO check not empty
    #print('Common wavelength range: {0} - {1}'.format(min(wavelengths), max(wavelengths)))

    #Use the common wavelengths to mask the inputs:
    a_water = sbc.spectra_apply_wavelength_mask(a_water, wavelengths)
    a_ph_star = sbc.spectra_apply_wavelength_mask(a_ph_star, wavelengths)
    for i, substrate in enumerate(substrates):
        substrates[i] = sbc.spectra_apply_wavelength_mask(
            substrate, wavelengths)

    print('awater: min: {0}  max: {1}'.format(min(a_water[0]),
                                              max(a_water[0])))
    print('a_ph_star: min: {0}  max: {1}'.format(min(a_ph_star[0]),
                                                 max(a_ph_star[0])))
    for substrate_name, substrate in zip(substrate_names, substrates):
        print('{0}: min: {1}  max: {2}'.format(substrate_name,
                                               min(substrate[0]),
                                               max(substrate[0])))
    """Truncate the sensor filter to match the common wavelength range
    It remains to be seen whether this is the best approach, but it works for this demo. An alternative approach would be to truncate the entire band for any band that falls outside the common wavelength range.
    If this approach, or something based on it, is valid, then this should be moved into a sambuca_core function with appropriate unit tests."""

    filter_mask = (sensor_filter[0] >=
                   wavelengths.min()) & (sensor_filter[0] <= wavelengths.max())
    sensor_filter = sensor_filter[0][filter_mask], sensor_filter[
        1][:, filter_mask]

    fixed_parameters = sb.create_fixed_parameter_set(
        wavelengths=wavelengths,
        a_water=a_water,
        a_ph_star=a_ph_star,
        substrates=substrates,
        sub1_frac=None,
        sub2_frac=None,
        sub3_frac=None,
        chl=None,
        cdom=None,
        nap=None,
        depth=None,
        a_cdom_slope=siop['a_cdom_slope'],
        a_nap_slope=siop['a_nap_slope'],
        bb_ph_slope=siop['bb_ph_slope'],
        bb_nap_slope=siop['bb_nap_slope'],
        lambda0cdom=siop['lambda0cdom'],
        lambda0nap=siop['lambda0nap'],
        lambda0x=siop['lambda0x'],
        x_ph_lambda0x=siop['x_ph_lambda0x'],
        x_nap_lambda0x=siop['x_nap_lambda0x'],
        a_cdom_lambda0cdom=siop['a_cdom_lambda0cdom'],
        a_nap_lambda0nap=siop['a_nap_lambda0nap'],
        bb_lambda_ref=siop['bb_lambda_ref'],
        water_refractive_index=siop['water_refractive_index'],
        theta_air=envmeta['theta_air'],
        off_nadir=envmeta['off_nadir'],
        q_factor=envmeta['q_factor'])
    result_recorder = sb.ArrayResultWriter(observed_rrs_height,
                                           observed_rrs_width, sensor_filter,
                                           nedr, fixed_parameters)
    error_dict = {
        'alpha': sb.distance_alpha,
        'alpha_f': sb.distance_alpha_f,
        'lsq': sb.distance_lsq,
        'f': sb.distance_f
    }
    objective = sb.SciPyObjective(
        sensor_filter,
        fixed_parameters,
        error_function=error_dict[error_name.lower()],
        nedr=nedr)
    siop['a_water'] = a_water
    siop['a_ph_star'] = a_ph_star
    siop['substrates'] = substrates
    siop['substrate_names'] = substrate_names
    image_info['sensor_filter'] = sensor_filter
    image_info['observed_rrs_width'] = observed_rrs_width
    image_info['observed_rrs_height'] = observed_rrs_height
    image_info['nedr'] = nedr

    #print ('EXIT PREPARE')

    return wavelengths, siop, image_info, fixed_parameters, result_recorder, objective
Example #3
0
    # In[92]:

    ##from IPython.display import clear_output, display
    ##from ipywidgets import IntProgress, Text
    ##
    ##progress_bar = IntProgress()
    ##text_widget = Text()
    ##skip_count_widget = Text()
    ##percentage_widget = Text()

    # ## Create the objective calculator

    # In[93]:

    objective = sb.SciPyObjective(sensor_filter,
                                  fixed_parameters,
                                  error_function=sb.distance_f,
                                  nedr=nedr)

    # ## Create the pixel result handler for capturing per-pixel outputs

    # In[94]:

    result_recorder = sb.ArrayResultWriter(observed_rrs_width,
                                           observed_rrs_height, sensor_filter,
                                           nedr, fixed_parameters)

    # ## Start some workers

    # In[95]:

    pool = None