def test_inc_coh_tmm():
    GaInP = material("GaInP")(In=0.5)
    GaAs = material("GaAs")()
    Ge = material("Ge")()

    optical_struct = SolarCell([
        Layer(material=GaInP, width=si("5000nm")),
        Layer(material=GaAs, width=si("200nm")),
        Layer(material=GaAs, width=si("5um")),
        Layer(material=Ge, width=si("50um")),
    ])

    wl = np.linspace(400, 1200, 5) * 1e-9

    options = State()
    options.wavelength = wl
    options.optics_method = "TMM"
    options.no_back_reflection = False
    options.BL_correction = True
    options.recalculate_absorption = True

    c_list = [
        ["c", "c", "c", "c"],
        ["c", "c", "c", "i"],
        ["c", "i", "i", "c"],
        ["i", "i", "i", "i"],
    ]

    results = []
    for i1, cl in enumerate(c_list):
        options.coherency_list = cl
        solar_cell_solver(optical_struct, "optics", options)
        results.append(optical_struct.absorbed)

    A_calc = np.stack(results)
    A_data = np.array(
        [[0.5742503, 0.67956899, 0.73481184, 0.725372, 0.76792856],
         [0.5742503, 0.67956899, 0.73481184, 0.725372, 0.76792856],
         [0.5742503, 0.67956899, 0.73474943, 0.70493469, 0.70361194],
         [0.5742503, 0.67956899, 0.70927724, 0.71509221, 0.71592772]])
    assert A_calc == approx(A_data)
Пример #2
0
    ],
             sn=1,
             sp=1,
             kind='DA')
]
# And, finally, we put everything together, adding also the surface recombination velocities sn and sp.
# setting kind = 'DA' in the Junction definition tells the electrical solver later to use the depletion approximation
optical_struct = SolarCell(ARC + top_junction + middle_junction + DBRa + DBRb +
                           DBRc + bottom_junction,
                           shading=0.05)

wl = np.linspace(250, 1700, 400) * 1e-9

options = State()
options.wavelength = wl
options.optics_method = 'TMM'
options.no_back_reflection = False
options.pol = 'p'
options.BL_correction = True
options.coherency_list = 111 * ['c']
options.theta = 30
solar_cell_solver(optical_struct, 'qe', options)

plt.figure()
plt.plot(
    wl * 1e9,
    optical_struct[0].layer_absorption + optical_struct[1].layer_absorption)
plt.plot(wl * 1e9, optical_struct[2].layer_absorption)
plt.plot(wl * 1e9, optical_struct[3].layer_absorption)
plt.plot(wl * 1e9, optical_struct[100].layer_absorption)
plt.plot(wl * 1e9, optical_struct.absorbed, '--')
Пример #3
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default_options.wavelength = np.linspace(300, 1800, 251) * 1e-9
default_options.light_source = LightSource(source_type='standard',
                                           version='AM1.5g',
                                           x=default_options.wavelength,
                                           output_units='photon_flux_per_m')

# IV control
default_options.voltages = np.linspace(0, 1.2, 100)
default_options.mpp = False
default_options.light_iv = False
default_options.internal_voltages = np.linspace(-6, 4, 1000)
default_options.position = None
default_options.radiative_coupling = False

# Optics control
default_options.optics_method = 'BL'
default_options.recalculate_absorption = False

default_options = merge_dicts(default_options, ASC.db_options, PDD.pdd_options,
                              rcwa_options)


def solar_cell_solver(solar_cell, task, user_options=None):
    """ Solves the properties of a solar cell object, either calculating its optical properties (R, A and T), its quantum efficiency or its current voltage characteristics in the dark or under illumination. The general options for the solvers are passed as dicionaries.

    :param solar_cell: A solar_cell object
    :param task: Task to perform. It has to be "optics", "iv", "qe", "equilibrium" or "short_circuit". The last two only work for PDD junctions
    :param user_options: A dictionary containing the options for the solver, which will overwrite the default options.
    :return: None
    """
    if type(user_options) in [State, dict]:
Пример #4
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    Layer(material=GaInP, width=si("5000nm")),
    Junction(
        [
            Layer(material=GaAs, width=si("200nm")),
            Layer(material=GaAs, width=si("5um")),
        ],
        kind="DA",
    ),
    Layer(material=Ge, width=si("50um")),
])

wl = np.linspace(250, 1700, 300) * 1e-9

options = State()
options.wavelength = wl
options.optics_method = "TMM"
options.no_back_reflection = False
options.BL_correction = True
options.recalculate_absorption = True
options.positions = [1e-8, 1e-9, 1e-8, 1e-7]
options.theta = 0

c_list = [
    ["c", "c", "c", "c"],
    ["c", "c", "c", "i"],
    ["c", "i", "i", "c"],
    ["i", "i", "i", "i"],
]

titles = [
    "All coherent",
ropt = dict(LatticeTruncation='Circular',
            DiscretizedEpsilon=True,
            DiscretizationResolution=4,
            PolarizationDecomposition=False,
            PolarizationBasis='Default',
            LanczosSmoothing=True,
            SubpixelSmoothing=True,
            ConserveMemory=False,
            WeismannFormulation=True)

light_source = LightSource(source_type='standard', version='AM0')

options = State()
options['rcwa_options'] = ropt
options.optics_method = 'RCWA'
options.wavelength = wavelengths
options.light_source = light_source
options.pol = 's'
options.mpp = True
options.light_iv = True
options.position = 1e-10
options.voltages = np.linspace(-1.5, 1.5, 100)
options.size = size
options.orders = 20
options.parallel = True

window_material = InGaP(In=0.485, Na=si(5e18, 'cm-3'))
# window_material.n_data = np.stack([wavelengths, InGaP_nk.n(wavelengths)])
# window_material.k_data = np.stack([wavelengths, InGaP_nk.k(wavelengths)])
# window_material.n_path = '/home/phoebe/Documents/rayflare/examples/data/InGaP_n.txt'