|
| 1 | +""" |
| 2 | +Modeling N. Martin and J. Ruiz Spectral Modifiers |
| 3 | +================================================= |
| 4 | +
|
| 5 | +Mimic Figures 4, 5 & 6 from paper [1]_. |
| 6 | +Note raw data is unavailable, so we are only plotting the line given from the |
| 7 | +model. |
| 8 | +
|
| 9 | +References |
| 10 | +---------- |
| 11 | +.. [1] Martín, N. and Ruiz, J.M. (1999), A new method for the spectral |
| 12 | + characterisation of PV modules. Prog. Photovolt: Res. Appl., 7: 299-310. |
| 13 | + :doi:10.1002/(SICI)1099-159X(199907/08)7:4<299::AID-PIP260>3.0.CO;2-0 |
| 14 | +""" |
| 15 | + |
| 16 | +from pvlib.spectrum.mismatch import martin_ruiz_spectral_modifier |
| 17 | +from pvlib.location import Location |
| 18 | +from pvlib.iotools import get_pvgis_tmy |
| 19 | +from pvlib.irradiance import get_extra_radiation, clearness_index |
| 20 | +from datetime import datetime, timedelta |
| 21 | +import numpy as np |
| 22 | +import pandas as pd |
| 23 | +import matplotlib.pyplot as plt |
| 24 | + |
| 25 | +# clearness_index = np.linspace(0.56, 0.82, 10) |
| 26 | + |
| 27 | +site = Location(40.4534, -3.7270, altitude=664, name='IES-UPM, Madrid') |
| 28 | + |
| 29 | +time = pd.date_range(start=datetime(2020, 1, 1), end=datetime(2020, 12, 31), |
| 30 | + freq=timedelta(hours=1)) |
| 31 | + |
| 32 | +tmy_data, _, _, _ = get_pvgis_tmy(site.latitude, site.longitude, |
| 33 | + map_variables=True) |
| 34 | +tmy_data = tmy_data.shift(freq=timedelta(minutes=-30)) |
| 35 | + |
| 36 | +solar_pos = site.get_solarposition(tmy_data.index) |
| 37 | + |
| 38 | +extra_rad = get_extra_radiation(tmy_data.index) |
| 39 | + |
| 40 | +clearness = clearness_index(ghi=tmy_data['ghi'], |
| 41 | + solar_zenith=solar_pos['zenith'], |
| 42 | + extra_radiation=extra_rad) |
| 43 | + |
| 44 | +print('clearness') |
| 45 | +print(clearness) |
| 46 | +clearness.plot() |
| 47 | + |
| 48 | +plt.show() |
| 49 | + |
| 50 | +print('pressure') |
| 51 | +pressure = site.get_airmass(model='kasten1966') |
| 52 | +print(pressure) |
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