solstice

Compute collected power and efficiencies of a solar plant
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solstice_sun_spectrum.h (1284B)

      1 /* Copyright (C) 2018-2026 |Meso|Star> (contact@meso-star.com)
      2  * Copyright (C) 2016-2018 CNRS
      3  *
      4  * This program is free software: you can redistribute it and/or modify
      5  * it under the terms of the GNU General Public License as published by
      6  * the Free Software Foundation, either version 3 of the License, or
      7  * (at your option) any later version.
      8  *
      9  * This program is distributed in the hope that it will be useful,
     10  * but WITHOUT ANY WARRANTY; without even the implied warranty of
     11  * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
     12  * GNU General Public License for more details.
     13  *
     14  * You should have received a copy of the GNU General Public License
     15  * along with this program. If not, see <http://www.gnu.org/licenses/>. */
     16 
     17 #ifndef SOLSTICE_SUN_SPECTRUM_H
     18 #define SOLSTICE_SUN_SPECTRUM_H
     19 
     20 #include <rsys/rsys.h>
     21 
     22 /*
     23  * Each built-in spectrum is a list of double2: [Wavelength in nano-meter,
     24  * DNI]. Its associated size is the number of double[2] into the spectrum
     25  */
     26 
     27 extern LOCAL_SYM const double solstice_sun_spectrum_dummy[];
     28 extern LOCAL_SYM const size_t solstice_sun_spectrum_dummy_size;
     29 
     30 extern LOCAL_SYM const double solstice_sun_spectrum_smarts[];
     31 extern LOCAL_SYM const size_t solstice_sun_spectrum_smarts_size;
     32 
     33 #endif /* SOLSTICE_SUN_SPECTRUM_H */
     34