示例#1
0
    def cloud_cover_to_irradiance_campbell_norman(self, cloud_cover, **kwargs):
        """
        Estimates irradiance from cloud cover in the following steps:

        1. Determine transmittance using a function of cloud cover e.g.
           :py:meth:`~ForecastModel.cloud_cover_to_transmittance_linear`
        2. Calculate GHI, DNI, DHI using the
           :py:func:`pvlib.irradiance.campbell_norman` model

        Parameters
        ----------
        cloud_cover : Series

        Returns
        -------
        irradiance : DataFrame
            Columns include ghi, dni, dhi
        """
        # in principle, get_solarposition could use the forecast
        # pressure, temp, etc., but the cloud cover forecast is not
        # accurate enough to justify using these minor corrections
        solar_position = self.location.get_solarposition(cloud_cover.index)
        dni_extra = get_extra_radiation(cloud_cover.index)

        transmittance = self.cloud_cover_to_transmittance_linear(
            cloud_cover, **kwargs)

        irrads = campbell_norman(solar_position['apparent_zenith'],
                                 transmittance,
                                 dni_extra=dni_extra)
        irrads = irrads.fillna(0)

        return irrads
示例#2
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def test_campbell_norman():
    expected = pd.DataFrame(np.array(
        [[863.859736967, 653.123094076, 220.65905025]]),
                            columns=['ghi', 'dni', 'dhi'],
                            index=[0])
    out = irradiance.campbell_norman(pd.Series([10]),
                                     pd.Series([0.5]),
                                     pd.Series([109764.21013135818]),
                                     dni_extra=1400)
    assert_frame_equal(out, expected)
def calculate_overcast_spectrl2():
    """
    This example will loop over a range of cloud covers and latitudes
    (at longitude=0) for a specific date and calculate the spectral
    irradiance with and without accounting for clouds. Clouds are accounted for
    by applying the cloud opacity factor defined in [1]. Several steps
    are required:
    1. Calculate the atmospheric and solar conditions for the
    location and time
    2. Calculate the spectral irradiance using `pvlib.spectrum.spectrl2`
    for clear sky conditions
    3. Calculate the dni, dhi, and ghi for cloudy conditions using
    `pvlib.irradiance.campbell_norman`
    4. Determine total in-plane irradiance and its beam,
    sky diffuse and ground
    reflected components for cloudy conditions -
    `pvlib.irradiance.get_total_irradiance`
    5. Calculate the dni, dhi, and ghi for clear sky conditions
    using `pvlib.irradiance.campbell_norman`
    6. Determine total in-plane irradiance and its beam,
    sky diffuse and ground
    reflected components for clear sky conditions -
    `pvlib.irradiance.get_total_irradiance`
    7. Calculate the cloud opacity factor [1] and scale the
    spectral results from step 4 - func cloud_opacity_factor
    8. Plot the results  - func plot_spectral_irradiance
    """
    month = 2
    hour_of_day = 12
    altitude = 0.0
    longitude = 0.0
    latitudes = [10, 40]

    # cloud cover in fraction units
    cloud_covers = [0.2, 0.5]
    water_vapor_content = 0.5
    tau500 = 0.1
    ground_albedo = 0.06
    ozone = 0.3
    surface_tilt = 0.0

    ctime, pv_system = setup_pv_system(month, hour_of_day)

    for cloud_cover in cloud_covers:
        for latitude in latitudes:
            sol = get_solarposition(ctime, latitude, longitude)
            az = sol['apparent_zenith'].to_numpy()
            airmass_relative = get_relative_airmass(az,
                                                    model='kastenyoung1989')
            pressure = pvlib.atmosphere.alt2pres(altitude)
            az = sol['apparent_zenith'].to_numpy()
            azimuth = sol['azimuth'].to_numpy()
            surface_azimuth = pv_system['surface_azimuth']

            transmittance = (1.0 - cloud_cover) * 0.75
            calc_aoi = aoi(surface_tilt, surface_azimuth, az, azimuth)

            # day of year is an int64index array so access first item
            day_of_year = ctime.dayofyear[0]

            spectra = pvlib.spectrum.spectrl2(
                apparent_zenith=az,
                aoi=calc_aoi,
                surface_tilt=surface_tilt,
                ground_albedo=ground_albedo,
                surface_pressure=pressure,
                relative_airmass=airmass_relative,
                precipitable_water=water_vapor_content,
                ozone=ozone,
                aerosol_turbidity_500nm=tau500,
                dayofyear=day_of_year)

            irrads_clouds = campbell_norman(sol['zenith'].to_numpy(),
                                            transmittance)

            # Convert the irradiance to a plane with tilt zero
            # horizontal to the earth. This is done applying
            #  tilt=0 to POA calculations using the output from
            # `campbell_norman`. The POA calculations include
            # calculating sky and ground diffuse light where
            # specific models can be selected (we use default).
            poa_irr_clouds = get_total_irradiance(
                surface_tilt=surface_tilt,
                surface_azimuth=pv_system['surface_azimuth'],
                dni=irrads_clouds['dni'],
                ghi=irrads_clouds['ghi'],
                dhi=irrads_clouds['dhi'],
                solar_zenith=sol['apparent_zenith'],
                solar_azimuth=sol['azimuth'])

            show_info(latitude, poa_irr_clouds)
            zen = sol['zenith'].to_numpy()
            irr_clearsky = campbell_norman(zen, transmittance=0.75)

            poa_irr_clearsky = get_total_irradiance(
                surface_tilt=surface_tilt,
                surface_azimuth=pv_system['surface_azimuth'],
                dni=irr_clearsky['dni'],
                ghi=irr_clearsky['ghi'],
                dhi=irr_clearsky['dhi'],
                solar_zenith=sol['apparent_zenith'],
                solar_azimuth=sol['azimuth'])

            show_info(latitude, poa_irr_clearsky)
            poa_dr = poa_irr_clouds['poa_direct'].values
            poa_diff = poa_irr_clouds['poa_diffuse'].values
            poa_global = poa_irr_clouds['poa_global'].values
            f_dir, f_diff = cloud_opacity_factor(poa_dr, poa_diff, poa_global,
                                                 spectra)

            plot_spectral_irr(spectra,
                              f_dir,
                              f_diff,
                              lat=latitude,
                              doy=day_of_year,
                              year=ctime.year[0],
                              clouds=cloud_cover)