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greg |
2.9 |
/* Copyright (c) 1994,2006 *Fraunhofer Institut for Solar Energy Systems
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* Heidenhofstr. 2, D-79110 Freiburg, Germany
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greg |
2.1 |
* *Agence de l'Environnement et de la Maitrise de l'Energie
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* Centre de Valbonne, 500 route des Lucioles, 06565 Sophia Antipolis Cedex, France
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* *BOUYGUES
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* 1 Avenue Eugene Freyssinet, Saint-Quentin-Yvelines, France
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*/
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#include <stdio.h>
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#include <string.h>
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| 11 |
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#include <math.h>
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#include <stdlib.h>
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#include "color.h"
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greg |
2.12 |
#include "sun.h"
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greg |
2.1 |
#include "paths.h"
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greg |
2.9 |
#define DOT(v1,v2) (v1[0]*v2[0]+v1[1]*v2[1]+v1[2]*v2[2])
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greg |
2.14 |
#define _USE_MATH_DEFINES
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greg |
2.1 |
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double normsc();
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greg |
2.14 |
/*static char *rcsid="$Header: /tmp_mnt/nfs/koll7/users/koll/jean/program/radiance/RAD/RCS/gendaylit.c,v 1.13 94/05/17 19:21:01 jean Exp Locker: jean $";*/
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greg |
2.9 |
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float coeff_perez[] = {
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greg |
2.12 |
1.3525,-0.2576,-0.2690,-1.4366,-0.7670,0.0007,1.2734,-0.1233,2.8000,0.6004,1.2375,1.000,1.8734,0.6297,
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0.9738,0.2809,0.0356,-0.1246,-0.5718,0.9938,-1.2219,-0.7730,1.4148,1.1016,-0.2054,0.0367,-3.9128,0.9156,
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6.9750,0.1774,6.4477,-0.1239,-1.5798,-0.5081,-1.7812,0.1080,0.2624,0.0672,-0.2190,-0.4285,-1.1000,-0.2515,
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0.8952,0.0156,0.2782,-0.1812,-4.5000,1.1766,24.7219,-13.0812,-37.7000,34.8438,-5.0000,1.5218,3.9229,
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-2.6204,-0.0156,0.1597,0.4199,-0.5562,-0.5484,-0.6654,-0.2672,0.7117,0.7234,-0.6219,-5.6812,2.6297,
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33.3389,-18.3000,-62.2500,52.0781,-3.5000,0.0016,1.1477,0.1062,0.4659,-0.3296,-0.0876,-0.0329,-0.6000,
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-0.3566,-2.5000,2.3250,0.2937,0.0496,-5.6812,1.8415,21.0000,-4.7656,-21.5906,7.2492,-3.5000,-0.1554,
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1.4062,0.3988,0.0032,0.0766,-0.0656,-0.1294,-1.0156,-0.3670,1.0078,1.4051,0.2875,-0.5328,-3.8500,3.3750,
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14.0000,-0.9999,-7.1406,7.5469,-3.4000,-0.1078,-1.0750,1.5702,-0.0672,0.4016,0.3017,-0.4844,-1.0000,
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0.0211,0.5025,-0.5119,-0.3000,0.1922,0.7023,-1.6317,19.0000,-5.0000,1.2438,-1.9094,-4.0000,0.0250,0.3844,
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0.2656,1.0468,-0.3788,-2.4517,1.4656,-1.0500,0.0289,0.4260,0.3590,-0.3250,0.1156,0.7781,0.0025,31.0625,
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-14.5000,-46.1148,55.3750,-7.2312,0.4050,13.3500,0.6234,1.5000,-0.6426,1.8564,0.5636};
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float defangle_theta[] = {
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84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84, 84,
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84, 84, 84, 84, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72, 72,
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72, 72, 72, 72, 72, 72, 72, 72, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60,
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60, 60, 60, 60, 60, 60, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48, 48,
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48, 48, 48, 48, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 36, 24, 24, 24, 24,
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24, 24, 24, 24, 24, 24, 24, 24, 12, 12, 12, 12, 12, 12, 0};
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float defangle_phi[] = {
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0, 12, 24, 36, 48, 60, 72, 84, 96, 108, 120, 132, 144, 156, 168, 180, 192, 204, 216, 228, 240, 252, 264,
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276, 288, 300, 312, 324, 336, 348, 0, 12, 24, 36, 48, 60, 72, 84, 96, 108, 120, 132, 144, 156, 168, 180,
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192, 204, 216, 228, 240, 252, 264, 276, 288, 300, 312, 324, 336, 348, 0, 15, 30, 45, 60, 75, 90, 105,
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120, 135, 150, 165, 180, 195, 210, 225, 240, 255, 270, 285, 300, 315, 330, 345, 0, 15, 30, 45, 60, 75,
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90, 105, 120, 135, 150, 165, 180, 195, 210, 225, 240, 255, 270, 285, 300, 315, 330, 345, 0, 20, 40, 60,
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80, 100, 120, 140, 160, 180, 200, 220, 240, 260, 280, 300, 320, 340, 0, 30, 60, 90, 120, 150, 180, 210,
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240, 270, 300, 330, 0, 60, 120, 180, 240, 300, 0};
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greg |
2.1 |
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greg |
2.14 |
/* Perez sky parametrization: epsilon and delta calculations from the direct and diffuse irradiances */
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greg |
2.1 |
double sky_brightness();
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double sky_clearness();
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/* calculation of the direct and diffuse components from the Perez parametrization */
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greg |
2.9 |
double diffuse_irradiance_from_sky_brightness();
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greg |
2.1 |
double direct_irradiance_from_sky_clearness();
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greg |
2.12 |
/* Perez global horizontal, diffuse horizontal and direct normal luminous efficacy models : */
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/* input w(cm)=2cm, solar zenith angle(degrees); output efficacy(lm/W) */
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greg |
2.1 |
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double glob_h_effi_PEREZ();
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double glob_h_diffuse_effi_PEREZ();
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double direct_n_effi_PEREZ();
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greg |
2.12 |
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greg |
2.1 |
/*likelihood check of the epsilon, delta, direct and diffuse components*/
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void check_parametrization();
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void check_irradiances();
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void check_illuminances();
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void illu_to_irra_index();
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greg |
2.9 |
void print_error_sky();
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greg |
2.1 |
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greg |
2.12 |
double calc_rel_lum_perez(double dzeta,double gamma,double Z,double epsilon,double Delta,float coeff_perez[]);
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greg |
2.9 |
void coeff_lum_perez(double Z, double epsilon, double Delta, float coeff_perez[]);
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greg |
2.1 |
double radians(double degres);
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double degres(double radians);
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void theta_phi_to_dzeta_gamma(double theta,double phi,double *dzeta,double *gamma, double Z);
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double integ_lv(float *lv,float *theta);
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greg |
2.9 |
void printdefaults();
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greg |
2.12 |
void check_sun_position();
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greg |
2.9 |
void computesky();
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void printhead(int ac, char** av);
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greg |
2.14 |
void usage_error(char* msg);
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greg |
2.9 |
void printsky();
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greg |
2.1 |
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greg |
2.9 |
FILE * frlibopen(char* fname);
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greg |
2.1 |
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/* astronomy and geometry*/
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double get_eccentricity();
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double air_mass();
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| 101 |
greg |
2.14 |
double solar_sunset(int month, int day);
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| 102 |
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double solar_sunrise(int month, int day);
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greg |
2.12 |
double stadj();
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int jdate(int month, int day);
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greg |
2.1 |
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/* sun calculation constants */
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greg |
2.12 |
extern double s_latitude;
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extern double s_longitude;
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extern double s_meridian;
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greg |
2.1 |
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const double AU = 149597890E3;
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const double solar_constant_e = 1367; /* solar constant W/m^2 */
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greg |
2.14 |
const double solar_constant_l = 127500; /* solar constant lux */
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greg |
2.1 |
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const double half_sun_angle = 0.2665;
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const double half_direct_angle = 2.85;
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| 118 |
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greg |
2.14 |
const double skyclearinf = 1.0; /* limitations for the variation of the Perez parameters */
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const double skyclearsup = 12.01;
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greg |
2.1 |
const double skybriginf = 0.01;
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const double skybrigsup = 0.6;
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/* required values */
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int month, day; /* date */
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double hour; /* time */
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int tsolar; /* 0=standard, 1=solar */
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double altitude, azimuth; /* or solar angles */
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| 134 |
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/* definition of the sky conditions through the Perez parametrization */
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greg |
2.9 |
double skyclearness = 0;
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double skybrightness = 0;
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greg |
2.12 |
double solarradiance;
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double diffuseilluminance, directilluminance, diffuseirradiance, directirradiance, globalirradiance;
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double sunzenith, daynumber, atm_preci_water=2;
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greg |
2.1 |
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greg |
2.12 |
/*double sunaltitude_border = 0;*/
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| 142 |
greg |
2.9 |
double diffnormalization = 0;
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| 143 |
greg |
2.12 |
double dirnormalization = 0;
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| 144 |
greg |
2.1 |
double *c_perez;
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| 145 |
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| 146 |
greg |
2.12 |
int output=0; /* define the unit of the output (sky luminance or radiance): */
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| 147 |
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/* visible watt=0, solar watt=1, lumen=2 */
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int input=0; /* define the input for the calulation */
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greg |
2.1 |
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| 150 |
greg |
2.9 |
int suppress_warnings=0;
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| 151 |
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greg |
2.1 |
/* default values */
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| 153 |
greg |
2.12 |
int cloudy = 0; /* 1=standard, 2=uniform */
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| 154 |
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int dosun = 1;
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| 155 |
greg |
2.1 |
double zenithbr = -1.0;
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| 156 |
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double betaturbidity = 0.1;
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| 157 |
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double gprefl = 0.2;
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| 158 |
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int S_INTER=0;
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| 159 |
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| 160 |
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/* computed values */
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| 161 |
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double sundir[3];
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| 162 |
greg |
2.9 |
double groundbr = 0;
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| 163 |
greg |
2.1 |
double F2;
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| 164 |
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double solarbr = 0.0;
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| 165 |
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int u_solar = 0; /* -1=irradiance, 1=radiance */
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| 166 |
greg |
2.12 |
float timeinterval = 0;
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| 167 |
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| 168 |
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char *progname;
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char errmsg[128];
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| 170 |
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| 171 |
greg |
2.14 |
double st;
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| 172 |
greg |
2.1 |
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| 173 |
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| 174 |
greg |
2.9 |
int main(int argc, char** argv)
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| 175 |
greg |
2.1 |
{
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| 176 |
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int i;
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| 177 |
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| 178 |
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progname = argv[0];
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| 179 |
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if (argc == 2 && !strcmp(argv[1], "-defaults")) {
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| 180 |
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printdefaults();
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| 181 |
greg |
2.9 |
return 0;
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| 182 |
greg |
2.1 |
}
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| 183 |
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if (argc < 4)
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| 184 |
greg |
2.14 |
usage_error("arg count");
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| 185 |
greg |
2.1 |
if (!strcmp(argv[1], "-ang")) {
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| 186 |
greg |
2.9 |
altitude = atof(argv[2]) * (M_PI/180);
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| 187 |
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azimuth = atof(argv[3]) * (M_PI/180);
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| 188 |
greg |
2.1 |
month = 0;
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| 189 |
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} else {
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| 190 |
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month = atoi(argv[1]);
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| 191 |
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if (month < 1 || month > 12)
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| 192 |
greg |
2.14 |
usage_error("bad month");
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| 193 |
greg |
2.1 |
day = atoi(argv[2]);
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| 194 |
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if (day < 1 || day > 31)
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| 195 |
greg |
2.14 |
usage_error("bad day");
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| 196 |
greg |
2.1 |
hour = atof(argv[3]);
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| 197 |
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if (hour < 0 || hour >= 24)
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| 198 |
greg |
2.14 |
usage_error("bad hour");
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| 199 |
greg |
2.1 |
tsolar = argv[3][0] == '+';
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| 200 |
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}
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| 201 |
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for (i = 4; i < argc; i++)
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| 202 |
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if (argv[i][0] == '-' || argv[i][0] == '+')
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| 203 |
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switch (argv[i][1]) {
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| 204 |
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case 's':
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| 205 |
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cloudy = 0;
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| 206 |
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dosun = argv[i][0] == '+';
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| 207 |
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break;
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| 208 |
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case 'R':
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| 209 |
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u_solar = argv[i][1] == 'R' ? -1 : 1;
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| 210 |
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solarbr = atof(argv[++i]);
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| 211 |
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break;
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| 212 |
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case 'c':
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| 213 |
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cloudy = argv[i][0] == '+' ? 2 : 1;
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| 214 |
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dosun = 0;
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| 215 |
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break;
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| 216 |
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case 't':
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| 217 |
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betaturbidity = atof(argv[++i]);
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| 218 |
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break;
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| 219 |
greg |
2.9 |
case 'w':
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| 220 |
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suppress_warnings = 1;
|
| 221 |
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break;
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| 222 |
greg |
2.1 |
case 'b':
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| 223 |
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zenithbr = atof(argv[++i]);
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| 224 |
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break;
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| 225 |
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case 'g':
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| 226 |
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gprefl = atof(argv[++i]);
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| 227 |
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break;
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| 228 |
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case 'a':
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| 229 |
greg |
2.9 |
s_latitude = atof(argv[++i]) * (M_PI/180);
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| 230 |
greg |
2.1 |
break;
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| 231 |
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case 'o':
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| 232 |
greg |
2.9 |
s_longitude = atof(argv[++i]) * (M_PI/180);
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| 233 |
greg |
2.1 |
break;
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| 234 |
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case 'm':
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| 235 |
greg |
2.9 |
s_meridian = atof(argv[++i]) * (M_PI/180);
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| 236 |
greg |
2.1 |
break;
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| 237 |
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|
| 238 |
|
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case 'O':
|
| 239 |
greg |
2.14 |
output = atof(argv[++i]); /*define the unit of the output of the program:
|
| 240 |
|
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sky and sun luminance/radiance
|
| 241 |
|
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(0==W visible, 1==W solar radiation, 2==lm) */
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| 242 |
greg |
2.1 |
break;
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| 243 |
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| 244 |
|
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case 'P':
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| 245 |
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input = 0; /* Perez parameters: epsilon, delta */
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| 246 |
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skyclearness = atof(argv[++i]);
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| 247 |
|
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skybrightness = atof(argv[++i]);
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| 248 |
|
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break;
|
| 249 |
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|
| 250 |
|
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case 'W': /* direct normal Irradiance [W/m^2] */
|
| 251 |
|
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input = 1; /* diffuse horizontal Irrad. [W/m^2] */
|
| 252 |
|
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directirradiance = atof(argv[++i]);
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| 253 |
greg |
2.9 |
diffuseirradiance = atof(argv[++i]);
|
| 254 |
greg |
2.1 |
break;
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| 255 |
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|
| 256 |
|
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case 'L': /* direct normal Illuminance [Lux] */
|
| 257 |
|
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input = 2; /* diffuse horizontal Ill. [Lux] */
|
| 258 |
|
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directilluminance = atof(argv[++i]);
|
| 259 |
greg |
2.9 |
diffuseilluminance = atof(argv[++i]);
|
| 260 |
greg |
2.1 |
break;
|
| 261 |
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| 262 |
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case 'G': /* direct horizontal Irradiance [W/m^2] */
|
| 263 |
|
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input = 3; /* diffuse horizontal Irrad. [W/m^2] */
|
| 264 |
|
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directirradiance = atof(argv[++i]);
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| 265 |
greg |
2.9 |
diffuseirradiance = atof(argv[++i]);
|
| 266 |
|
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break;
|
| 267 |
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|
| 268 |
greg |
2.12 |
case 'E': /* Erbs model based on the */
|
| 269 |
|
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input = 4; /* global-horizontal irradiance [W/m^2] */
|
| 270 |
|
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globalirradiance = atof(argv[++i]);
|
| 271 |
|
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break;
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| 272 |
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| 273 |
|
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case 'i':
|
| 274 |
|
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timeinterval = atof(argv[++i]);
|
| 275 |
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break;
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| 276 |
greg |
2.9 |
|
| 277 |
greg |
2.1 |
|
| 278 |
|
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default:
|
| 279 |
|
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sprintf(errmsg, "unknown option: %s", argv[i]);
|
| 280 |
greg |
2.14 |
usage_error(errmsg);
|
| 281 |
greg |
2.1 |
}
|
| 282 |
|
|
else
|
| 283 |
greg |
2.14 |
usage_error("bad option");
|
| 284 |
greg |
2.1 |
|
| 285 |
greg |
2.14 |
if (month && !tsolar && fabs(s_meridian-s_longitude) > 45*M_PI/180)
|
| 286 |
|
|
fprintf(stderr,"%s: warning: %.1f hours btwn. standard meridian and longitude\n",
|
| 287 |
greg |
2.9 |
progname, (s_longitude-s_meridian)*12/M_PI);
|
| 288 |
greg |
2.1 |
|
| 289 |
|
|
|
| 290 |
greg |
2.12 |
/* dynamic memory allocation for the pointers */
|
| 291 |
greg |
2.9 |
if ( (c_perez = calloc(5, sizeof(double))) == NULL )
|
| 292 |
greg |
2.14 |
{ fprintf(stderr,"Out of memory error in function main"); return 1; }
|
| 293 |
greg |
2.1 |
|
| 294 |
greg |
2.14 |
|
| 295 |
greg |
2.1 |
printhead(argc, argv);
|
| 296 |
|
|
computesky();
|
| 297 |
|
|
printsky();
|
| 298 |
greg |
2.9 |
return 0;
|
| 299 |
greg |
2.14 |
|
| 300 |
greg |
2.1 |
}
|
| 301 |
|
|
|
| 302 |
|
|
|
| 303 |
greg |
2.12 |
|
| 304 |
|
|
|
| 305 |
|
|
|
| 306 |
|
|
void computesky()
|
| 307 |
greg |
2.1 |
{
|
| 308 |
|
|
|
| 309 |
greg |
2.6 |
int j;
|
| 310 |
greg |
2.12 |
|
| 311 |
|
|
float *lv_mod; /* 145 luminance values */
|
| 312 |
greg |
2.9 |
float *theta_o, *phi_o;
|
| 313 |
greg |
2.1 |
double dzeta, gamma;
|
| 314 |
|
|
double normfactor;
|
| 315 |
greg |
2.12 |
double erbs_s0, erbs_kt;
|
| 316 |
greg |
2.1 |
|
| 317 |
|
|
|
| 318 |
|
|
/* compute solar direction */
|
| 319 |
greg |
2.12 |
|
| 320 |
greg |
2.1 |
if (month) { /* from date and time */
|
| 321 |
|
|
int jd;
|
| 322 |
greg |
2.14 |
double sd;
|
| 323 |
greg |
2.1 |
|
| 324 |
|
|
jd = jdate(month, day); /* Julian date */
|
| 325 |
|
|
sd = sdec(jd); /* solar declination */
|
| 326 |
|
|
if (tsolar) /* solar time */
|
| 327 |
|
|
st = hour;
|
| 328 |
|
|
else
|
| 329 |
|
|
st = hour + stadj(jd);
|
| 330 |
greg |
2.12 |
|
| 331 |
|
|
|
| 332 |
|
|
if(timeinterval) {
|
| 333 |
|
|
|
| 334 |
|
|
if(timeinterval<0) {
|
| 335 |
|
|
fprintf(stderr, "time interval negative\n");
|
| 336 |
|
|
exit(1);
|
| 337 |
|
|
}
|
| 338 |
greg |
2.14 |
|
| 339 |
|
|
if(fabs(solar_sunrise(month,day)-st)<=timeinterval/120) {
|
| 340 |
|
|
st= (st+timeinterval/120+solar_sunrise(month,day))/2;
|
| 341 |
|
|
if(suppress_warnings==0)
|
| 342 |
|
|
{ fprintf(stderr, "Solar position corrected at time step %d %d %.3f\n",month,day,hour); }
|
| 343 |
greg |
2.12 |
}
|
| 344 |
|
|
|
| 345 |
greg |
2.14 |
if(fabs(solar_sunset(month,day)-st)<timeinterval/120) {
|
| 346 |
|
|
st= (st-timeinterval/120+solar_sunset(month,day))/2;
|
| 347 |
|
|
if(suppress_warnings==0)
|
| 348 |
|
|
{ fprintf(stderr, "Solar position corrected at time step %d %d %.3f\n",month,day,hour); }
|
| 349 |
greg |
2.12 |
}
|
| 350 |
greg |
2.14 |
|
| 351 |
|
|
if((st<solar_sunrise(month,day)-timeinterval/120) || (st>solar_sunset(month,day)+timeinterval/120)) {
|
| 352 |
|
|
if(suppress_warnings==0)
|
| 353 |
|
|
{ fprintf(stderr, "Warning: sun position too low, printing error sky at %d %d %.3f\n",month,day,hour); }
|
| 354 |
|
|
altitude = salt(sd, st);
|
| 355 |
|
|
azimuth = sazi(sd, st);
|
| 356 |
|
|
print_error_sky();
|
| 357 |
|
|
exit(0);
|
| 358 |
|
|
}
|
| 359 |
greg |
2.12 |
}
|
| 360 |
greg |
2.14 |
else
|
| 361 |
greg |
2.12 |
|
| 362 |
greg |
2.14 |
if(st<solar_sunrise(month,day) || st>solar_sunset(month,day)) {
|
| 363 |
|
|
if(suppress_warnings==0)
|
| 364 |
|
|
{ fprintf(stderr, "Warning: sun altitude below zero at time step %i %i %.2f, printing error sky\n",month,day,hour); }
|
| 365 |
|
|
altitude = salt(sd, st);
|
| 366 |
|
|
azimuth = sazi(sd, st);
|
| 367 |
|
|
print_error_sky();
|
| 368 |
|
|
exit(0);
|
| 369 |
|
|
}
|
| 370 |
greg |
2.12 |
|
| 371 |
greg |
2.1 |
altitude = salt(sd, st);
|
| 372 |
|
|
azimuth = sazi(sd, st);
|
| 373 |
|
|
|
| 374 |
|
|
daynumber = (double)jdate(month, day);
|
| 375 |
greg |
2.12 |
|
| 376 |
greg |
2.1 |
}
|
| 377 |
greg |
2.9 |
|
| 378 |
|
|
|
| 379 |
greg |
2.12 |
|
| 380 |
|
|
|
| 381 |
greg |
2.9 |
|
| 382 |
|
|
if (!cloudy && altitude > 87.*M_PI/180.) {
|
| 383 |
|
|
|
| 384 |
|
|
if (suppress_warnings==0) {
|
| 385 |
|
|
fprintf(stderr,
|
| 386 |
greg |
2.1 |
"%s: warning - sun too close to zenith, reducing altitude to 87 degrees\n",
|
| 387 |
|
|
progname);
|
| 388 |
greg |
2.9 |
}
|
| 389 |
|
|
altitude = 87.*M_PI/180.;
|
| 390 |
greg |
2.1 |
}
|
| 391 |
greg |
2.9 |
|
| 392 |
greg |
2.14 |
|
| 393 |
|
|
|
| 394 |
greg |
2.1 |
sundir[0] = -sin(azimuth)*cos(altitude);
|
| 395 |
|
|
sundir[1] = -cos(azimuth)*cos(altitude);
|
| 396 |
|
|
sundir[2] = sin(altitude);
|
| 397 |
|
|
|
| 398 |
|
|
|
| 399 |
|
|
/* calculation for the new functions */
|
| 400 |
greg |
2.9 |
sunzenith = 90 - altitude*180/M_PI;
|
| 401 |
greg |
2.14 |
|
| 402 |
greg |
2.1 |
|
| 403 |
greg |
2.9 |
/* compute the inputs for the calculation of the light distribution over the sky*/
|
| 404 |
greg |
2.12 |
if (input==0) /* P */
|
| 405 |
greg |
2.1 |
{
|
| 406 |
|
|
check_parametrization();
|
| 407 |
greg |
2.9 |
diffuseirradiance = diffuse_irradiance_from_sky_brightness(); /*diffuse horizontal irradiance*/
|
| 408 |
greg |
2.1 |
directirradiance = direct_irradiance_from_sky_clearness();
|
| 409 |
|
|
check_irradiances();
|
| 410 |
|
|
|
| 411 |
|
|
if (output==0 || output==2)
|
| 412 |
|
|
{
|
| 413 |
greg |
2.9 |
diffuseilluminance = diffuseirradiance*glob_h_diffuse_effi_PEREZ();/*diffuse horizontal illuminance*/
|
| 414 |
greg |
2.1 |
directilluminance = directirradiance*direct_n_effi_PEREZ();
|
| 415 |
|
|
check_illuminances();
|
| 416 |
|
|
}
|
| 417 |
|
|
}
|
| 418 |
|
|
|
| 419 |
|
|
|
| 420 |
greg |
2.12 |
else if (input==1) /* W */
|
| 421 |
greg |
2.1 |
{
|
| 422 |
|
|
check_irradiances();
|
| 423 |
|
|
skybrightness = sky_brightness();
|
| 424 |
|
|
skyclearness = sky_clearness();
|
| 425 |
greg |
2.14 |
|
| 426 |
greg |
2.1 |
check_parametrization();
|
| 427 |
greg |
2.14 |
|
| 428 |
greg |
2.1 |
if (output==0 || output==2)
|
| 429 |
|
|
{
|
| 430 |
greg |
2.9 |
diffuseilluminance = diffuseirradiance*glob_h_diffuse_effi_PEREZ();/*diffuse horizontal illuminance*/
|
| 431 |
greg |
2.1 |
directilluminance = directirradiance*direct_n_effi_PEREZ();
|
| 432 |
|
|
check_illuminances();
|
| 433 |
|
|
}
|
| 434 |
|
|
|
| 435 |
|
|
}
|
| 436 |
|
|
|
| 437 |
|
|
|
| 438 |
greg |
2.12 |
else if (input==2) /* L */
|
| 439 |
greg |
2.1 |
{
|
| 440 |
|
|
check_illuminances();
|
| 441 |
|
|
illu_to_irra_index();
|
| 442 |
|
|
check_parametrization();
|
| 443 |
|
|
}
|
| 444 |
|
|
|
| 445 |
|
|
|
| 446 |
greg |
2.12 |
else if (input==3) /* G */
|
| 447 |
greg |
2.1 |
{
|
| 448 |
|
|
if (altitude<=0)
|
| 449 |
|
|
{
|
| 450 |
greg |
2.9 |
if (suppress_warnings==0)
|
| 451 |
greg |
2.14 |
fprintf(stderr, "Warning: sun altitude < 0, proceed with irradiance values of zero\n");
|
| 452 |
greg |
2.9 |
directirradiance = 0;
|
| 453 |
|
|
diffuseirradiance = 0;
|
| 454 |
|
|
} else {
|
| 455 |
greg |
2.12 |
|
| 456 |
|
|
directirradiance=directirradiance/sin(altitude);
|
| 457 |
greg |
2.1 |
}
|
| 458 |
greg |
2.12 |
|
| 459 |
greg |
2.1 |
check_irradiances();
|
| 460 |
|
|
skybrightness = sky_brightness();
|
| 461 |
|
|
skyclearness = sky_clearness();
|
| 462 |
|
|
check_parametrization();
|
| 463 |
|
|
|
| 464 |
|
|
if (output==0 || output==2)
|
| 465 |
|
|
{
|
| 466 |
greg |
2.9 |
diffuseilluminance = diffuseirradiance*glob_h_diffuse_effi_PEREZ();/*diffuse horizontal illuminance*/
|
| 467 |
greg |
2.1 |
directilluminance = directirradiance*direct_n_effi_PEREZ();
|
| 468 |
|
|
check_illuminances();
|
| 469 |
|
|
}
|
| 470 |
|
|
|
| 471 |
|
|
}
|
| 472 |
|
|
|
| 473 |
greg |
2.12 |
|
| 474 |
|
|
else if (input==4) /* E */ /* Implementation of the Erbs model. W.Sprenger (04/13) */
|
| 475 |
|
|
{
|
| 476 |
|
|
|
| 477 |
|
|
if (altitude<=0)
|
| 478 |
|
|
{
|
| 479 |
|
|
if (suppress_warnings==0 && globalirradiance > 50)
|
| 480 |
|
|
fprintf(stderr, "Warning: global irradiance higher than 50 W/m^2 while the sun altitude is lower than zero\n");
|
| 481 |
|
|
globalirradiance = 0; diffuseirradiance = 0; directirradiance = 0;
|
| 482 |
|
|
|
| 483 |
|
|
} else {
|
| 484 |
|
|
|
| 485 |
|
|
erbs_s0 = solar_constant_e*get_eccentricity()*sin(altitude);
|
| 486 |
|
|
|
| 487 |
|
|
if (globalirradiance>erbs_s0)
|
| 488 |
|
|
{
|
| 489 |
|
|
if (suppress_warnings==0)
|
| 490 |
|
|
fprintf(stderr, "Warning: global irradiance is higher than the time-dependent solar constant s0\n");
|
| 491 |
|
|
globalirradiance=erbs_s0*0.999;
|
| 492 |
|
|
}
|
| 493 |
|
|
|
| 494 |
|
|
erbs_kt=globalirradiance/erbs_s0;
|
| 495 |
|
|
|
| 496 |
|
|
if (erbs_kt<=0.22) diffuseirradiance=globalirradiance*(1-0.09*erbs_kt);
|
| 497 |
|
|
else if (erbs_kt<=0.8) diffuseirradiance=globalirradiance*(0.9511-0.1604*erbs_kt+4.388*pow(erbs_kt,2)-16.638*pow(erbs_kt,3)+12.336*pow(erbs_kt,4));
|
| 498 |
|
|
else if (erbs_kt<1) diffuseirradiance=globalirradiance*(0.165);
|
| 499 |
|
|
|
| 500 |
|
|
directirradiance=globalirradiance-diffuseirradiance;
|
| 501 |
|
|
|
| 502 |
|
|
printf("# erbs_s0, erbs_kt, irr_dir_h, irr_diff: %.3f %.3f %.3f %.3f\n", erbs_s0, erbs_kt, directirradiance, diffuseirradiance);
|
| 503 |
greg |
2.14 |
printf("# WARNING: the -E option is only recommended for a rough estimation!\n");
|
| 504 |
greg |
2.12 |
|
| 505 |
|
|
directirradiance=directirradiance/sin(altitude);
|
| 506 |
|
|
|
| 507 |
|
|
}
|
| 508 |
|
|
|
| 509 |
|
|
check_irradiances();
|
| 510 |
|
|
skybrightness = sky_brightness();
|
| 511 |
|
|
skyclearness = sky_clearness();
|
| 512 |
|
|
check_parametrization();
|
| 513 |
|
|
|
| 514 |
|
|
if (output==0 || output==2)
|
| 515 |
|
|
{
|
| 516 |
|
|
diffuseilluminance = diffuseirradiance*glob_h_diffuse_effi_PEREZ();/*diffuse horizontal illuminance*/
|
| 517 |
|
|
directilluminance = directirradiance*direct_n_effi_PEREZ();
|
| 518 |
|
|
check_illuminances();
|
| 519 |
|
|
}
|
| 520 |
|
|
|
| 521 |
|
|
}
|
| 522 |
|
|
|
| 523 |
|
|
|
| 524 |
|
|
|
| 525 |
greg |
2.1 |
|
| 526 |
greg |
2.14 |
else { fprintf(stderr,"error at the input arguments"); exit(1); }
|
| 527 |
greg |
2.1 |
|
| 528 |
|
|
|
| 529 |
|
|
|
| 530 |
greg |
2.9 |
/* normalization factor for the relative sky luminance distribution, diffuse part*/
|
| 531 |
greg |
2.12 |
|
| 532 |
greg |
2.1 |
if ( (lv_mod = malloc(145*sizeof(float))) == NULL)
|
| 533 |
|
|
{
|
| 534 |
|
|
fprintf(stderr,"Out of memory in function main");
|
| 535 |
|
|
exit(1);
|
| 536 |
|
|
}
|
| 537 |
|
|
|
| 538 |
|
|
/* read the angles */
|
| 539 |
greg |
2.9 |
theta_o = defangle_theta;
|
| 540 |
|
|
phi_o = defangle_phi;
|
| 541 |
greg |
2.12 |
|
| 542 |
greg |
2.1 |
|
| 543 |
greg |
2.9 |
/* parameters for the perez model */
|
| 544 |
greg |
2.1 |
coeff_lum_perez(radians(sunzenith), skyclearness, skybrightness, coeff_perez);
|
| 545 |
|
|
|
| 546 |
greg |
2.12 |
|
| 547 |
|
|
|
| 548 |
greg |
2.9 |
/*calculation of the modelled luminance */
|
| 549 |
greg |
2.1 |
for (j=0;j<145;j++)
|
| 550 |
|
|
{
|
| 551 |
|
|
theta_phi_to_dzeta_gamma(radians(*(theta_o+j)),radians(*(phi_o+j)),&dzeta,&gamma,radians(sunzenith));
|
| 552 |
greg |
2.12 |
|
| 553 |
greg |
2.1 |
*(lv_mod+j) = calc_rel_lum_perez(dzeta,gamma,radians(sunzenith),skyclearness,skybrightness,coeff_perez);
|
| 554 |
greg |
2.12 |
|
| 555 |
|
|
/* fprintf(stderr,"theta, phi, lv_mod %f\t %f\t %f\n", *(theta_o+j),*(phi_o+j),*(lv_mod+j)); */
|
| 556 |
greg |
2.1 |
}
|
| 557 |
greg |
2.12 |
|
| 558 |
greg |
2.1 |
/* integration of luminance for the normalization factor, diffuse part of the sky*/
|
| 559 |
greg |
2.12 |
|
| 560 |
greg |
2.1 |
diffnormalization = integ_lv(lv_mod, theta_o);
|
| 561 |
|
|
|
| 562 |
|
|
|
| 563 |
|
|
|
| 564 |
greg |
2.9 |
/*normalization coefficient in lumen or in watt*/
|
| 565 |
greg |
2.1 |
if (output==0)
|
| 566 |
|
|
{
|
| 567 |
greg |
2.9 |
diffnormalization = diffuseilluminance/diffnormalization/WHTEFFICACY;
|
| 568 |
greg |
2.1 |
}
|
| 569 |
|
|
else if (output==1)
|
| 570 |
|
|
{
|
| 571 |
greg |
2.9 |
diffnormalization = diffuseirradiance/diffnormalization;
|
| 572 |
greg |
2.1 |
}
|
| 573 |
|
|
else if (output==2)
|
| 574 |
|
|
{
|
| 575 |
greg |
2.9 |
diffnormalization = diffuseilluminance/diffnormalization;
|
| 576 |
greg |
2.1 |
}
|
| 577 |
|
|
|
| 578 |
greg |
2.9 |
else {fprintf(stderr,"Wrong output specification.\n"); exit(1);}
|
| 579 |
greg |
2.1 |
|
| 580 |
|
|
|
| 581 |
|
|
|
| 582 |
|
|
|
| 583 |
greg |
2.9 |
/* calculation for the solar source */
|
| 584 |
greg |
2.1 |
if (output==0)
|
| 585 |
greg |
2.9 |
solarradiance = directilluminance/(2*M_PI*(1-cos(half_sun_angle*M_PI/180)))/WHTEFFICACY;
|
| 586 |
greg |
2.1 |
|
| 587 |
|
|
else if (output==1)
|
| 588 |
greg |
2.9 |
solarradiance = directirradiance/(2*M_PI*(1-cos(half_sun_angle*M_PI/180)));
|
| 589 |
greg |
2.1 |
|
| 590 |
|
|
else
|
| 591 |
greg |
2.9 |
solarradiance = directilluminance/(2*M_PI*(1-cos(half_sun_angle*M_PI/180)));
|
| 592 |
greg |
2.1 |
|
| 593 |
|
|
|
| 594 |
|
|
|
| 595 |
greg |
2.14 |
/* Compute the ground radiance */
|
| 596 |
|
|
zenithbr=calc_rel_lum_perez(0.0,radians(sunzenith),radians(sunzenith),skyclearness,skybrightness,coeff_perez);
|
| 597 |
|
|
zenithbr*=diffnormalization;
|
| 598 |
greg |
2.9 |
|
| 599 |
greg |
2.14 |
if (skyclearness==1)
|
| 600 |
greg |
2.1 |
normfactor = 0.777778;
|
| 601 |
|
|
|
| 602 |
greg |
2.14 |
if (skyclearness>=6)
|
| 603 |
greg |
2.1 |
{
|
| 604 |
greg |
2.9 |
F2 = 0.274*(0.91 + 10.0*exp(-3.0*(M_PI/2.0-altitude)) + 0.45*sundir[2]*sundir[2]);
|
| 605 |
|
|
normfactor = normsc()/F2/M_PI;
|
| 606 |
greg |
2.1 |
}
|
| 607 |
|
|
|
| 608 |
greg |
2.14 |
if ( (skyclearness>1) && (skyclearness<6) )
|
| 609 |
greg |
2.1 |
{
|
| 610 |
|
|
S_INTER=1;
|
| 611 |
greg |
2.9 |
F2 = (2.739 + .9891*sin(.3119+2.6*altitude)) * exp(-(M_PI/2.0-altitude)*(.4441+1.48*altitude));
|
| 612 |
|
|
normfactor = normsc()/F2/M_PI;
|
| 613 |
greg |
2.1 |
}
|
| 614 |
|
|
|
| 615 |
greg |
2.14 |
groundbr = zenithbr*normfactor;
|
| 616 |
greg |
2.1 |
|
| 617 |
greg |
2.14 |
if (dosun&&(skyclearness>1))
|
| 618 |
greg |
2.9 |
groundbr += 6.8e-5/M_PI*solarradiance*sundir[2];
|
| 619 |
greg |
2.1 |
|
| 620 |
greg |
2.14 |
groundbr *= gprefl;
|
| 621 |
greg |
2.1 |
|
| 622 |
|
|
|
| 623 |
greg |
2.14 |
|
| 624 |
|
|
if(*(c_perez+1)>0)
|
| 625 |
|
|
{
|
| 626 |
|
|
if(suppress_warnings==0)
|
| 627 |
|
|
{ fprintf(stderr, "Warning: positive Perez parameter B (= %lf), printing error sky\n",*(c_perez+1));}
|
| 628 |
|
|
print_error_sky();
|
| 629 |
|
|
exit(0);
|
| 630 |
|
|
}
|
| 631 |
|
|
|
| 632 |
greg |
2.1 |
|
| 633 |
|
|
return;
|
| 634 |
|
|
}
|
| 635 |
|
|
|
| 636 |
|
|
|
| 637 |
|
|
|
| 638 |
|
|
|
| 639 |
greg |
2.12 |
|
| 640 |
|
|
double solar_sunset(int month,int day)
|
| 641 |
|
|
{
|
| 642 |
|
|
float W;
|
| 643 |
|
|
extern double s_latitude;
|
| 644 |
|
|
W=-1*(tan(s_latitude)*tan(sdec(jdate(month, day))));
|
| 645 |
|
|
return(12+(M_PI/2 - atan2(W,sqrt(1-W*W)))*180/(M_PI*15));
|
| 646 |
|
|
}
|
| 647 |
|
|
|
| 648 |
|
|
|
| 649 |
greg |
2.14 |
|
| 650 |
|
|
|
| 651 |
greg |
2.12 |
double solar_sunrise(int month,int day)
|
| 652 |
|
|
{
|
| 653 |
|
|
float W;
|
| 654 |
|
|
extern double s_latitude;
|
| 655 |
|
|
W=-1*(tan(s_latitude)*tan(sdec(jdate(month, day))));
|
| 656 |
|
|
return(12-(M_PI/2 - atan2(W,sqrt(1-W*W)))*180/(M_PI*15));
|
| 657 |
|
|
}
|
| 658 |
|
|
|
| 659 |
|
|
|
| 660 |
|
|
|
| 661 |
|
|
|
| 662 |
greg |
2.14 |
void printsky()
|
| 663 |
|
|
{
|
| 664 |
|
|
|
| 665 |
|
|
printf("# Local solar time: %.2f\n", st);
|
| 666 |
|
|
printf("# Solar altitude and azimuth: %.1f %.1f\n", altitude*180/M_PI, azimuth*180/M_PI);
|
| 667 |
greg |
2.12 |
|
| 668 |
|
|
|
| 669 |
greg |
2.1 |
if (dosun&&(skyclearness>1))
|
| 670 |
greg |
2.9 |
{
|
| 671 |
greg |
2.1 |
printf("\nvoid light solar\n");
|
| 672 |
|
|
printf("0\n0\n");
|
| 673 |
|
|
printf("3 %.3e %.3e %.3e\n", solarradiance, solarradiance, solarradiance);
|
| 674 |
|
|
printf("\nsolar source sun\n");
|
| 675 |
|
|
printf("0\n0\n");
|
| 676 |
|
|
printf("4 %f %f %f %f\n", sundir[0], sundir[1], sundir[2], 2*half_sun_angle);
|
| 677 |
greg |
2.9 |
} else if (dosun) {
|
| 678 |
greg |
2.1 |
printf("\nvoid light solar\n");
|
| 679 |
|
|
printf("0\n0\n");
|
| 680 |
|
|
printf("3 0.0 0.0 0.0\n");
|
| 681 |
|
|
printf("\nsolar source sun\n");
|
| 682 |
|
|
printf("0\n0\n");
|
| 683 |
|
|
printf("4 %f %f %f %f\n", sundir[0], sundir[1], sundir[2], 2*half_sun_angle);
|
| 684 |
greg |
2.9 |
}
|
| 685 |
greg |
2.1 |
|
| 686 |
greg |
2.12 |
|
| 687 |
greg |
2.1 |
printf("\nvoid brightfunc skyfunc\n");
|
| 688 |
|
|
printf("2 skybright perezlum.cal\n");
|
| 689 |
|
|
printf("0\n");
|
| 690 |
|
|
printf("10 %.3e %.3e %lf %lf %lf %lf %lf %f %f %f \n", diffnormalization, groundbr,
|
| 691 |
greg |
2.9 |
*(c_perez+0),*(c_perez+1),*(c_perez+2),*(c_perez+3),*(c_perez+4),
|
| 692 |
|
|
sundir[0], sundir[1], sundir[2]);
|
| 693 |
greg |
2.12 |
|
| 694 |
greg |
2.1 |
}
|
| 695 |
|
|
|
| 696 |
|
|
|
| 697 |
greg |
2.14 |
|
| 698 |
|
|
void print_error_sky()
|
| 699 |
|
|
{
|
| 700 |
|
|
|
| 701 |
|
|
|
| 702 |
|
|
sundir[0] = -sin(azimuth)*cos(altitude);
|
| 703 |
|
|
sundir[1] = -cos(azimuth)*cos(altitude);
|
| 704 |
|
|
sundir[2] = sin(altitude);
|
| 705 |
|
|
|
| 706 |
|
|
printf("# Local solar time: %.2f\n", st);
|
| 707 |
|
|
printf("# Solar altitude and azimuth: %.1f %.1f\n", altitude*180/M_PI, azimuth*180/M_PI);
|
| 708 |
|
|
|
| 709 |
|
|
printf("\nvoid brightfunc skyfunc\n");
|
| 710 |
|
|
printf("2 skybright perezlum.cal\n");
|
| 711 |
|
|
printf("0\n");
|
| 712 |
|
|
printf("10 0.00 0.00 0.000 0.000 0.000 0.000 0.000 %f %f %f \n", sundir[0], sundir[1], sundir[2]);
|
| 713 |
|
|
}
|
| 714 |
|
|
|
| 715 |
|
|
|
| 716 |
|
|
|
| 717 |
|
|
|
| 718 |
|
|
|
| 719 |
greg |
2.9 |
void printdefaults() /* print default values */
|
| 720 |
greg |
2.1 |
{
|
| 721 |
|
|
printf("-g %f\t\t\t# Ground plane reflectance\n", gprefl);
|
| 722 |
|
|
if (zenithbr > 0.0)
|
| 723 |
|
|
printf("-b %f\t\t\t# Zenith radiance (watts/ster/m^2\n", zenithbr);
|
| 724 |
|
|
else
|
| 725 |
|
|
printf("-t %f\t\t\t# Atmospheric betaturbidity\n", betaturbidity);
|
| 726 |
greg |
2.9 |
printf("-a %f\t\t\t# Site latitude (degrees)\n", s_latitude*(180/M_PI));
|
| 727 |
|
|
printf("-o %f\t\t\t# Site longitude (degrees)\n", s_longitude*(180/M_PI));
|
| 728 |
|
|
printf("-m %f\t\t\t# Standard meridian (degrees)\n", s_meridian*(180/M_PI));
|
| 729 |
greg |
2.1 |
}
|
| 730 |
|
|
|
| 731 |
|
|
|
| 732 |
greg |
2.14 |
|
| 733 |
|
|
|
| 734 |
|
|
void usage_error(char* msg) /* print usage error and quit */
|
| 735 |
greg |
2.1 |
{
|
| 736 |
|
|
if (msg != NULL)
|
| 737 |
greg |
2.12 |
fprintf(stderr, "%s: Use error - %s\n\n", progname, msg);
|
| 738 |
|
|
fprintf(stderr, "Usage: %s month day hour [...]\n", progname);
|
| 739 |
|
|
fprintf(stderr, " or: %s -ang altitude azimuth [...]\n", progname);
|
| 740 |
|
|
fprintf(stderr, " followed by: -P epsilon delta [options]\n");
|
| 741 |
|
|
fprintf(stderr, " or: [-W|-L|-G] direct_value diffuse_value [options]\n");
|
| 742 |
|
|
fprintf(stderr, " or: -E global_irradiance [options]\n\n");
|
| 743 |
|
|
fprintf(stderr, " Description:\n");
|
| 744 |
greg |
2.1 |
fprintf(stderr, " -P epsilon delta (these are the Perez parameters) \n");
|
| 745 |
|
|
fprintf(stderr, " -W direct-normal-irradiance diffuse-horizontal-irradiance (W/m^2)\n");
|
| 746 |
|
|
fprintf(stderr, " -L direct-normal-illuminance diffuse-horizontal-illuminance (lux)\n");
|
| 747 |
|
|
fprintf(stderr, " -G direct-horizontal-irradiance diffuse-horizontal-irradiance (W/m^2)\n");
|
| 748 |
greg |
2.12 |
fprintf(stderr, " -E global-horizontal-irradiance (W/m^2)\n\n");
|
| 749 |
|
|
fprintf(stderr, " Output specification with option:\n");
|
| 750 |
greg |
2.1 |
fprintf(stderr, " -O [0|1|2] (0=output in W/m^2/sr visible, 1=output in W/m^2/sr solar, 2=output in candela/m^2), default is 0 \n");
|
| 751 |
greg |
2.14 |
fprintf(stderr, " gendaylit version 2.4 (2013/09/04) \n\n");
|
| 752 |
greg |
2.1 |
exit(1);
|
| 753 |
|
|
}
|
| 754 |
|
|
|
| 755 |
|
|
|
| 756 |
|
|
|
| 757 |
greg |
2.14 |
|
| 758 |
greg |
2.9 |
double normsc() /* compute normalization factor (E0*F2/L0) */
|
| 759 |
greg |
2.1 |
{
|
| 760 |
|
|
static double nfc[2][5] = {
|
| 761 |
|
|
/* clear sky approx. */
|
| 762 |
|
|
{2.766521, 0.547665, -0.369832, 0.009237, 0.059229},
|
| 763 |
|
|
/* intermediate sky approx. */
|
| 764 |
|
|
{3.5556, -2.7152, -1.3081, 1.0660, 0.60227},
|
| 765 |
|
|
};
|
| 766 |
|
|
register double *nf;
|
| 767 |
|
|
double x, nsc;
|
| 768 |
|
|
register int i;
|
| 769 |
|
|
/* polynomial approximation */
|
| 770 |
|
|
nf = nfc[S_INTER];
|
| 771 |
greg |
2.9 |
x = (altitude - M_PI/4.0)/(M_PI/4.0);
|
| 772 |
greg |
2.1 |
nsc = nf[i=4];
|
| 773 |
|
|
while (i--)
|
| 774 |
|
|
nsc = nsc*x + nf[i];
|
| 775 |
|
|
|
| 776 |
|
|
return(nsc);
|
| 777 |
|
|
}
|
| 778 |
|
|
|
| 779 |
|
|
|
| 780 |
|
|
|
| 781 |
greg |
2.14 |
|
| 782 |
|
|
|
| 783 |
greg |
2.9 |
void printhead(int ac, char** av) /* print command header */
|
| 784 |
greg |
2.1 |
{
|
| 785 |
|
|
putchar('#');
|
| 786 |
|
|
while (ac--) {
|
| 787 |
|
|
putchar(' ');
|
| 788 |
|
|
fputs(*av++, stdout);
|
| 789 |
|
|
}
|
| 790 |
|
|
putchar('\n');
|
| 791 |
|
|
}
|
| 792 |
|
|
|
| 793 |
|
|
|
| 794 |
|
|
|
| 795 |
|
|
|
| 796 |
greg |
2.14 |
|
| 797 |
|
|
|
| 798 |
greg |
2.1 |
/* Perez models */
|
| 799 |
|
|
|
| 800 |
|
|
/* Perez global horizontal luminous efficacy model */
|
| 801 |
|
|
double glob_h_effi_PEREZ()
|
| 802 |
|
|
{
|
| 803 |
|
|
|
| 804 |
|
|
double value;
|
| 805 |
|
|
double category_bounds[10], a[10], b[10], c[10], d[10];
|
| 806 |
|
|
int category_total_number, category_number, i;
|
| 807 |
greg |
2.12 |
|
| 808 |
|
|
check_parametrization();
|
| 809 |
|
|
|
| 810 |
|
|
|
| 811 |
|
|
/*if ((skyclearness<skyclearinf || skyclearness>skyclearsup || skybrightness<skybriginf || skybrightness>skybrigsup) && suppress_warnings==0)
|
| 812 |
|
|
fprintf(stderr, "Warning: skyclearness or skybrightness out of range in function glob_h_effi_PEREZ \n"); */
|
| 813 |
|
|
|
| 814 |
|
|
|
| 815 |
greg |
2.1 |
/* initialize category bounds (clearness index bounds) */
|
| 816 |
|
|
|
| 817 |
|
|
category_total_number = 8;
|
| 818 |
|
|
|
| 819 |
|
|
category_bounds[1] = 1;
|
| 820 |
|
|
category_bounds[2] = 1.065;
|
| 821 |
|
|
category_bounds[3] = 1.230;
|
| 822 |
|
|
category_bounds[4] = 1.500;
|
| 823 |
|
|
category_bounds[5] = 1.950;
|
| 824 |
|
|
category_bounds[6] = 2.800;
|
| 825 |
|
|
category_bounds[7] = 4.500;
|
| 826 |
|
|
category_bounds[8] = 6.200;
|
| 827 |
|
|
category_bounds[9] = 12.01;
|
| 828 |
|
|
|
| 829 |
|
|
|
| 830 |
|
|
/* initialize model coefficients */
|
| 831 |
|
|
a[1] = 96.63;
|
| 832 |
|
|
a[2] = 107.54;
|
| 833 |
|
|
a[3] = 98.73;
|
| 834 |
|
|
a[4] = 92.72;
|
| 835 |
|
|
a[5] = 86.73;
|
| 836 |
|
|
a[6] = 88.34;
|
| 837 |
|
|
a[7] = 78.63;
|
| 838 |
|
|
a[8] = 99.65;
|
| 839 |
|
|
|
| 840 |
|
|
b[1] = -0.47;
|
| 841 |
|
|
b[2] = 0.79;
|
| 842 |
|
|
b[3] = 0.70;
|
| 843 |
|
|
b[4] = 0.56;
|
| 844 |
|
|
b[5] = 0.98;
|
| 845 |
|
|
b[6] = 1.39;
|
| 846 |
|
|
b[7] = 1.47;
|
| 847 |
|
|
b[8] = 1.86;
|
| 848 |
|
|
|
| 849 |
|
|
c[1] = 11.50;
|
| 850 |
|
|
c[2] = 1.79;
|
| 851 |
|
|
c[3] = 4.40;
|
| 852 |
|
|
c[4] = 8.36;
|
| 853 |
|
|
c[5] = 7.10;
|
| 854 |
|
|
c[6] = 6.06;
|
| 855 |
|
|
c[7] = 4.93;
|
| 856 |
|
|
c[8] = -4.46;
|
| 857 |
|
|
|
| 858 |
|
|
d[1] = -9.16;
|
| 859 |
|
|
d[2] = -1.19;
|
| 860 |
|
|
d[3] = -6.95;
|
| 861 |
|
|
d[4] = -8.31;
|
| 862 |
|
|
d[5] = -10.94;
|
| 863 |
|
|
d[6] = -7.60;
|
| 864 |
|
|
d[7] = -11.37;
|
| 865 |
|
|
d[8] = -3.15;
|
| 866 |
|
|
|
| 867 |
|
|
|
| 868 |
|
|
|
| 869 |
|
|
for (i=1; i<=category_total_number; i++)
|
| 870 |
|
|
{
|
| 871 |
|
|
if ( (skyclearness >= category_bounds[i]) && (skyclearness < category_bounds[i+1]) )
|
| 872 |
|
|
category_number = i;
|
| 873 |
|
|
}
|
| 874 |
|
|
|
| 875 |
|
|
value = a[category_number] + b[category_number]*atm_preci_water +
|
| 876 |
greg |
2.9 |
c[category_number]*cos(sunzenith*M_PI/180) + d[category_number]*log(skybrightness);
|
| 877 |
greg |
2.1 |
|
| 878 |
|
|
return(value);
|
| 879 |
|
|
}
|
| 880 |
|
|
|
| 881 |
|
|
|
| 882 |
greg |
2.14 |
|
| 883 |
|
|
|
| 884 |
greg |
2.1 |
/* global horizontal diffuse efficacy model, according to PEREZ */
|
| 885 |
|
|
double glob_h_diffuse_effi_PEREZ()
|
| 886 |
|
|
{
|
| 887 |
|
|
double value;
|
| 888 |
|
|
double category_bounds[10], a[10], b[10], c[10], d[10];
|
| 889 |
|
|
int category_total_number, category_number, i;
|
| 890 |
|
|
|
| 891 |
greg |
2.12 |
check_parametrization();
|
| 892 |
greg |
2.1 |
|
| 893 |
greg |
2.12 |
|
| 894 |
|
|
/*if ((skyclearness<skyclearinf || skyclearness>skyclearsup || skybrightness<skybriginf || skybrightness>skybrigsup) && suppress_warnings==0)
|
| 895 |
greg |
2.14 |
fprintf(stderr, "Warning: skyclearness or skybrightness out of range in function glob_h_diffuse_PEREZ \n"); */
|
| 896 |
greg |
2.12 |
|
| 897 |
greg |
2.1 |
/* initialize category bounds (clearness index bounds) */
|
| 898 |
|
|
|
| 899 |
|
|
category_total_number = 8;
|
| 900 |
|
|
|
| 901 |
greg |
2.12 |
//XXX: category_bounds > 0.1
|
| 902 |
greg |
2.1 |
category_bounds[1] = 1;
|
| 903 |
|
|
category_bounds[2] = 1.065;
|
| 904 |
|
|
category_bounds[3] = 1.230;
|
| 905 |
|
|
category_bounds[4] = 1.500;
|
| 906 |
|
|
category_bounds[5] = 1.950;
|
| 907 |
|
|
category_bounds[6] = 2.800;
|
| 908 |
|
|
category_bounds[7] = 4.500;
|
| 909 |
|
|
category_bounds[8] = 6.200;
|
| 910 |
|
|
category_bounds[9] = 12.01;
|
| 911 |
|
|
|
| 912 |
|
|
|
| 913 |
|
|
/* initialize model coefficients */
|
| 914 |
|
|
a[1] = 97.24;
|
| 915 |
|
|
a[2] = 107.22;
|
| 916 |
|
|
a[3] = 104.97;
|
| 917 |
|
|
a[4] = 102.39;
|
| 918 |
|
|
a[5] = 100.71;
|
| 919 |
|
|
a[6] = 106.42;
|
| 920 |
|
|
a[7] = 141.88;
|
| 921 |
|
|
a[8] = 152.23;
|
| 922 |
|
|
|
| 923 |
|
|
b[1] = -0.46;
|
| 924 |
|
|
b[2] = 1.15;
|
| 925 |
|
|
b[3] = 2.96;
|
| 926 |
|
|
b[4] = 5.59;
|
| 927 |
|
|
b[5] = 5.94;
|
| 928 |
|
|
b[6] = 3.83;
|
| 929 |
|
|
b[7] = 1.90;
|
| 930 |
|
|
b[8] = 0.35;
|
| 931 |
|
|
|
| 932 |
|
|
c[1] = 12.00;
|
| 933 |
|
|
c[2] = 0.59;
|
| 934 |
|
|
c[3] = -5.53;
|
| 935 |
|
|
c[4] = -13.95;
|
| 936 |
|
|
c[5] = -22.75;
|
| 937 |
|
|
c[6] = -36.15;
|
| 938 |
|
|
c[7] = -53.24;
|
| 939 |
|
|
c[8] = -45.27;
|
| 940 |
|
|
|
| 941 |
|
|
d[1] = -8.91;
|
| 942 |
|
|
d[2] = -3.95;
|
| 943 |
|
|
d[3] = -8.77;
|
| 944 |
|
|
d[4] = -13.90;
|
| 945 |
|
|
d[5] = -23.74;
|
| 946 |
|
|
d[6] = -28.83;
|
| 947 |
|
|
d[7] = -14.03;
|
| 948 |
|
|
d[8] = -7.98;
|
| 949 |
|
|
|
| 950 |
|
|
|
| 951 |
|
|
|
| 952 |
greg |
2.9 |
category_number = -1;
|
| 953 |
greg |
2.1 |
for (i=1; i<=category_total_number; i++)
|
| 954 |
|
|
{
|
| 955 |
|
|
if ( (skyclearness >= category_bounds[i]) && (skyclearness < category_bounds[i+1]) )
|
| 956 |
|
|
category_number = i;
|
| 957 |
|
|
}
|
| 958 |
|
|
|
| 959 |
greg |
2.9 |
if (category_number == -1) {
|
| 960 |
|
|
if (suppress_warnings==0)
|
| 961 |
greg |
2.14 |
fprintf(stderr, "Warning: sky clearness (= %.3f) too high, printing error sky\n", skyclearness);
|
| 962 |
greg |
2.9 |
print_error_sky();
|
| 963 |
greg |
2.14 |
exit(0);
|
| 964 |
greg |
2.9 |
}
|
| 965 |
|
|
|
| 966 |
|
|
|
| 967 |
|
|
value = a[category_number] + b[category_number]*atm_preci_water + c[category_number]*cos(sunzenith*M_PI/180) +
|
| 968 |
greg |
2.1 |
d[category_number]*log(skybrightness);
|
| 969 |
|
|
|
| 970 |
|
|
return(value);
|
| 971 |
greg |
2.12 |
|
| 972 |
greg |
2.1 |
}
|
| 973 |
|
|
|
| 974 |
|
|
|
| 975 |
greg |
2.12 |
|
| 976 |
greg |
2.14 |
|
| 977 |
|
|
|
| 978 |
|
|
|
| 979 |
greg |
2.1 |
/* direct normal efficacy model, according to PEREZ */
|
| 980 |
|
|
|
| 981 |
|
|
double direct_n_effi_PEREZ()
|
| 982 |
|
|
|
| 983 |
|
|
{
|
| 984 |
|
|
double value;
|
| 985 |
|
|
double category_bounds[10], a[10], b[10], c[10], d[10];
|
| 986 |
|
|
int category_total_number, category_number, i;
|
| 987 |
|
|
|
| 988 |
|
|
|
| 989 |
greg |
2.14 |
/*if ((skyclearness<skyclearinf || skyclearness>skyclearsup || skybrightness<skybriginf || skybrightness>skybrigsup) && suppress_warnings==0)
|
| 990 |
|
|
fprintf(stderr, "Warning: skyclearness or skybrightness out of range in function direct_n_effi_PEREZ \n");*/
|
| 991 |
greg |
2.1 |
|
| 992 |
|
|
|
| 993 |
|
|
/* initialize category bounds (clearness index bounds) */
|
| 994 |
|
|
|
| 995 |
|
|
category_total_number = 8;
|
| 996 |
|
|
|
| 997 |
|
|
category_bounds[1] = 1;
|
| 998 |
|
|
category_bounds[2] = 1.065;
|
| 999 |
|
|
category_bounds[3] = 1.230;
|
| 1000 |
|
|
category_bounds[4] = 1.500;
|
| 1001 |
|
|
category_bounds[5] = 1.950;
|
| 1002 |
|
|
category_bounds[6] = 2.800;
|
| 1003 |
|
|
category_bounds[7] = 4.500;
|
| 1004 |
|
|
category_bounds[8] = 6.200;
|
| 1005 |
|
|
category_bounds[9] = 12.1;
|
| 1006 |
|
|
|
| 1007 |
|
|
|
| 1008 |
|
|
/* initialize model coefficients */
|
| 1009 |
|
|
a[1] = 57.20;
|
| 1010 |
|
|
a[2] = 98.99;
|
| 1011 |
|
|
a[3] = 109.83;
|
| 1012 |
|
|
a[4] = 110.34;
|
| 1013 |
|
|
a[5] = 106.36;
|
| 1014 |
|
|
a[6] = 107.19;
|
| 1015 |
|
|
a[7] = 105.75;
|
| 1016 |
|
|
a[8] = 101.18;
|
| 1017 |
|
|
|
| 1018 |
|
|
b[1] = -4.55;
|
| 1019 |
|
|
b[2] = -3.46;
|
| 1020 |
|
|
b[3] = -4.90;
|
| 1021 |
|
|
b[4] = -5.84;
|
| 1022 |
|
|
b[5] = -3.97;
|
| 1023 |
|
|
b[6] = -1.25;
|
| 1024 |
|
|
b[7] = 0.77;
|
| 1025 |
|
|
b[8] = 1.58;
|
| 1026 |
|
|
|
| 1027 |
|
|
c[1] = -2.98;
|
| 1028 |
|
|
c[2] = -1.21;
|
| 1029 |
|
|
c[3] = -1.71;
|
| 1030 |
|
|
c[4] = -1.99;
|
| 1031 |
|
|
c[5] = -1.75;
|
| 1032 |
|
|
c[6] = -1.51;
|
| 1033 |
|
|
c[7] = -1.26;
|
| 1034 |
|
|
c[8] = -1.10;
|
| 1035 |
|
|
|
| 1036 |
|
|
d[1] = 117.12;
|
| 1037 |
|
|
d[2] = 12.38;
|
| 1038 |
|
|
d[3] = -8.81;
|
| 1039 |
|
|
d[4] = -4.56;
|
| 1040 |
|
|
d[5] = -6.16;
|
| 1041 |
|
|
d[6] = -26.73;
|
| 1042 |
|
|
d[7] = -34.44;
|
| 1043 |
|
|
d[8] = -8.29;
|
| 1044 |
|
|
|
| 1045 |
|
|
|
| 1046 |
|
|
|
| 1047 |
|
|
for (i=1; i<=category_total_number; i++)
|
| 1048 |
|
|
{
|
| 1049 |
|
|
if ( (skyclearness >= category_bounds[i]) && (skyclearness < category_bounds[i+1]) )
|
| 1050 |
|
|
category_number = i;
|
| 1051 |
|
|
}
|
| 1052 |
|
|
|
| 1053 |
greg |
2.9 |
value = a[category_number] + b[category_number]*atm_preci_water + c[category_number]*exp(5.73*sunzenith*M_PI/180 - 5) + d[category_number]*skybrightness;
|
| 1054 |
greg |
2.1 |
|
| 1055 |
|
|
if (value < 0) value = 0;
|
| 1056 |
|
|
|
| 1057 |
|
|
return(value);
|
| 1058 |
|
|
}
|
| 1059 |
|
|
|
| 1060 |
|
|
|
| 1061 |
|
|
/*check the range of epsilon and delta indexes of the perez parametrization*/
|
| 1062 |
|
|
void check_parametrization()
|
| 1063 |
|
|
{
|
| 1064 |
greg |
2.14 |
|
| 1065 |
greg |
2.9 |
if (skyclearness<skyclearinf || skyclearness>skyclearsup || skybrightness<skybriginf || skybrightness>skybrigsup)
|
| 1066 |
greg |
2.1 |
{
|
| 1067 |
greg |
2.9 |
|
| 1068 |
|
|
/* limit sky clearness or sky brightness, 2009 11 13 by J. Wienold */
|
| 1069 |
greg |
2.14 |
|
| 1070 |
greg |
2.9 |
if (skyclearness<skyclearinf){
|
| 1071 |
greg |
2.14 |
/* if (suppress_warnings==0)
|
| 1072 |
|
|
fprintf(stderr,"Range warning: sky clearness too low (%lf)\n", skyclearness); */
|
| 1073 |
greg |
2.9 |
skyclearness=skyclearinf;
|
| 1074 |
|
|
}
|
| 1075 |
|
|
if (skyclearness>skyclearsup){
|
| 1076 |
greg |
2.14 |
/* if (suppress_warnings==0)
|
| 1077 |
|
|
fprintf(stderr,"Range warning: sky clearness too high (%lf)\n", skyclearness); */
|
| 1078 |
|
|
skyclearness=skyclearsup-0.001;
|
| 1079 |
greg |
2.9 |
}
|
| 1080 |
|
|
if (skybrightness<skybriginf){
|
| 1081 |
greg |
2.14 |
/* if (suppress_warnings==0)
|
| 1082 |
|
|
fprintf(stderr,"Range warning: sky brightness too low (%lf)\n", skybrightness); */
|
| 1083 |
greg |
2.9 |
skybrightness=skybriginf;
|
| 1084 |
|
|
}
|
| 1085 |
|
|
if (skybrightness>skybrigsup){
|
| 1086 |
greg |
2.14 |
/* if (suppress_warnings==0)
|
| 1087 |
|
|
fprintf(stderr,"Range warning: sky brightness too high (%lf)\n", skybrightness); */
|
| 1088 |
greg |
2.9 |
skybrightness=skybrigsup;
|
| 1089 |
greg |
2.1 |
}
|
| 1090 |
greg |
2.9 |
|
| 1091 |
|
|
return; }
|
| 1092 |
greg |
2.1 |
else return;
|
| 1093 |
|
|
}
|
| 1094 |
|
|
|
| 1095 |
|
|
|
| 1096 |
greg |
2.14 |
|
| 1097 |
|
|
|
| 1098 |
|
|
|
| 1099 |
greg |
2.9 |
/* validity of the direct and diffuse components */
|
| 1100 |
greg |
2.1 |
void check_illuminances()
|
| 1101 |
|
|
{
|
| 1102 |
greg |
2.9 |
if (directilluminance < 0) {
|
| 1103 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1104 |
|
|
{ fprintf(stderr,"Warning: direct illuminance < 0. Using 0.0\n"); }
|
| 1105 |
greg |
2.9 |
directilluminance = 0.0;
|
| 1106 |
|
|
}
|
| 1107 |
|
|
if (diffuseilluminance < 0) {
|
| 1108 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1109 |
|
|
{ fprintf(stderr,"Warning: diffuse illuminance < 0. Using 0.0\n"); }
|
| 1110 |
greg |
2.9 |
diffuseilluminance = 0.0;
|
| 1111 |
|
|
}
|
| 1112 |
greg |
2.14 |
|
| 1113 |
|
|
if (directilluminance+diffuseilluminance==0 && altitude > 0) {
|
| 1114 |
|
|
if(suppress_warnings==0)
|
| 1115 |
|
|
{ fprintf(stderr,"Warning: zero illuminance at sun altitude > 0, printing error sky\n"); }
|
| 1116 |
|
|
print_error_sky();
|
| 1117 |
|
|
exit(0);
|
| 1118 |
|
|
}
|
| 1119 |
|
|
|
| 1120 |
|
|
if (directilluminance > solar_constant_l) {
|
| 1121 |
|
|
if(suppress_warnings==0)
|
| 1122 |
|
|
{ fprintf(stderr,"Warning: direct illuminance exceeds solar constant\n"); }
|
| 1123 |
|
|
print_error_sky();
|
| 1124 |
|
|
exit(0);
|
| 1125 |
greg |
2.1 |
}
|
| 1126 |
|
|
}
|
| 1127 |
|
|
|
| 1128 |
|
|
|
| 1129 |
|
|
void check_irradiances()
|
| 1130 |
|
|
{
|
| 1131 |
greg |
2.9 |
if (directirradiance < 0) {
|
| 1132 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1133 |
|
|
{ fprintf(stderr,"Warning: direct irradiance < 0. Using 0.0\n"); }
|
| 1134 |
greg |
2.9 |
directirradiance = 0.0;
|
| 1135 |
|
|
}
|
| 1136 |
|
|
if (diffuseirradiance < 0) {
|
| 1137 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1138 |
|
|
{ fprintf(stderr,"Warning: diffuse irradiance < 0. Using 0.0\n"); }
|
| 1139 |
greg |
2.9 |
diffuseirradiance = 0.0;
|
| 1140 |
|
|
}
|
| 1141 |
greg |
2.14 |
|
| 1142 |
|
|
if (directirradiance+diffuseirradiance==0 && altitude > 0) {
|
| 1143 |
|
|
if(suppress_warnings==0)
|
| 1144 |
|
|
{ fprintf(stderr,"Warning: zero irradiance at sun altitude > 0, printing error sky\n"); }
|
| 1145 |
|
|
print_error_sky();
|
| 1146 |
|
|
exit(0);
|
| 1147 |
|
|
}
|
| 1148 |
|
|
|
| 1149 |
greg |
2.9 |
if (directirradiance > solar_constant_e) {
|
| 1150 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1151 |
|
|
{ fprintf(stderr,"Warning: direct irradiance exceeds solar constant\n"); }
|
| 1152 |
|
|
print_error_sky();
|
| 1153 |
|
|
exit(0);
|
| 1154 |
greg |
2.9 |
}
|
| 1155 |
greg |
2.1 |
}
|
| 1156 |
|
|
|
| 1157 |
|
|
|
| 1158 |
|
|
|
| 1159 |
|
|
/* Perez sky's brightness */
|
| 1160 |
|
|
double sky_brightness()
|
| 1161 |
|
|
{
|
| 1162 |
|
|
double value;
|
| 1163 |
|
|
|
| 1164 |
greg |
2.9 |
value = diffuseirradiance * air_mass() / ( solar_constant_e*get_eccentricity());
|
| 1165 |
greg |
2.1 |
|
| 1166 |
|
|
return(value);
|
| 1167 |
|
|
}
|
| 1168 |
|
|
|
| 1169 |
|
|
|
| 1170 |
|
|
/* Perez sky's clearness */
|
| 1171 |
|
|
double sky_clearness()
|
| 1172 |
|
|
{
|
| 1173 |
greg |
2.9 |
double value;
|
| 1174 |
greg |
2.1 |
|
| 1175 |
greg |
2.9 |
value = ( (diffuseirradiance + directirradiance)/(diffuseirradiance) + 1.041*sunzenith*M_PI/180*sunzenith*M_PI/180*sunzenith*M_PI/180 ) / (1 + 1.041*sunzenith*M_PI/180*sunzenith*M_PI/180*sunzenith*M_PI/180) ;
|
| 1176 |
greg |
2.1 |
|
| 1177 |
greg |
2.9 |
return(value);
|
| 1178 |
greg |
2.1 |
}
|
| 1179 |
|
|
|
| 1180 |
|
|
|
| 1181 |
|
|
|
| 1182 |
|
|
/* diffus horizontal irradiance from Perez sky's brightness */
|
| 1183 |
greg |
2.9 |
double diffuse_irradiance_from_sky_brightness()
|
| 1184 |
greg |
2.1 |
{
|
| 1185 |
|
|
double value;
|
| 1186 |
|
|
|
| 1187 |
|
|
value = skybrightness / air_mass() * ( solar_constant_e*get_eccentricity());
|
| 1188 |
|
|
|
| 1189 |
|
|
return(value);
|
| 1190 |
|
|
}
|
| 1191 |
|
|
|
| 1192 |
|
|
|
| 1193 |
|
|
/* direct normal irradiance from Perez sky's clearness */
|
| 1194 |
|
|
double direct_irradiance_from_sky_clearness()
|
| 1195 |
|
|
{
|
| 1196 |
|
|
double value;
|
| 1197 |
|
|
|
| 1198 |
greg |
2.9 |
value = diffuse_irradiance_from_sky_brightness();
|
| 1199 |
|
|
value = value * ( (skyclearness-1) * (1+1.041*sunzenith*M_PI/180*sunzenith*M_PI/180*sunzenith*M_PI/180) );
|
| 1200 |
greg |
2.1 |
|
| 1201 |
|
|
return(value);
|
| 1202 |
|
|
}
|
| 1203 |
|
|
|
| 1204 |
|
|
|
| 1205 |
greg |
2.12 |
|
| 1206 |
|
|
|
| 1207 |
greg |
2.9 |
void illu_to_irra_index()
|
| 1208 |
greg |
2.1 |
{
|
| 1209 |
greg |
2.9 |
double test1=0.1, test2=0.1, d_eff;
|
| 1210 |
greg |
2.1 |
int counter=0;
|
| 1211 |
|
|
|
| 1212 |
greg |
2.14 |
diffuseirradiance = diffuseilluminance*solar_constant_e/(solar_constant_l);
|
| 1213 |
|
|
directirradiance = directilluminance*solar_constant_e/(solar_constant_l);
|
| 1214 |
greg |
2.1 |
skyclearness = sky_clearness();
|
| 1215 |
|
|
skybrightness = sky_brightness();
|
| 1216 |
greg |
2.9 |
check_parametrization();
|
| 1217 |
greg |
2.12 |
|
| 1218 |
|
|
|
| 1219 |
greg |
2.9 |
while ( ((fabs(diffuseirradiance-test1)>10) || (fabs(directirradiance-test2)>10)
|
| 1220 |
greg |
2.12 |
|| (!(skyclearness<skyclearinf || skyclearness>skyclearsup))
|
| 1221 |
|
|
|| (!(skybrightness<skybriginf || skybrightness>skybrigsup)) )
|
| 1222 |
|
|
&& !(counter==9) )
|
| 1223 |
greg |
2.1 |
{
|
| 1224 |
greg |
2.12 |
|
| 1225 |
greg |
2.9 |
test1=diffuseirradiance;
|
| 1226 |
greg |
2.1 |
test2=directirradiance;
|
| 1227 |
|
|
counter++;
|
| 1228 |
|
|
|
| 1229 |
greg |
2.9 |
diffuseirradiance = diffuseilluminance/glob_h_diffuse_effi_PEREZ();
|
| 1230 |
|
|
d_eff = direct_n_effi_PEREZ();
|
| 1231 |
greg |
2.12 |
|
| 1232 |
|
|
|
| 1233 |
greg |
2.9 |
if (d_eff < 0.1)
|
| 1234 |
|
|
directirradiance = 0;
|
| 1235 |
greg |
2.12 |
else
|
| 1236 |
greg |
2.9 |
directirradiance = directilluminance/d_eff;
|
| 1237 |
greg |
2.1 |
|
| 1238 |
|
|
skybrightness = sky_brightness();
|
| 1239 |
|
|
skyclearness = sky_clearness();
|
| 1240 |
greg |
2.9 |
check_parametrization();
|
| 1241 |
greg |
2.12 |
|
| 1242 |
greg |
2.1 |
}
|
| 1243 |
|
|
|
| 1244 |
|
|
|
| 1245 |
|
|
return;
|
| 1246 |
|
|
}
|
| 1247 |
|
|
|
| 1248 |
greg |
2.9 |
static int get_numlin(float epsilon)
|
| 1249 |
greg |
2.1 |
{
|
| 1250 |
greg |
2.9 |
if (epsilon < 1.065)
|
| 1251 |
|
|
return 0;
|
| 1252 |
|
|
else if (epsilon < 1.230)
|
| 1253 |
|
|
return 1;
|
| 1254 |
|
|
else if (epsilon < 1.500)
|
| 1255 |
|
|
return 2;
|
| 1256 |
|
|
else if (epsilon < 1.950)
|
| 1257 |
|
|
return 3;
|
| 1258 |
|
|
else if (epsilon < 2.800)
|
| 1259 |
|
|
return 4;
|
| 1260 |
|
|
else if (epsilon < 4.500)
|
| 1261 |
|
|
return 5;
|
| 1262 |
|
|
else if (epsilon < 6.200)
|
| 1263 |
|
|
return 6;
|
| 1264 |
|
|
return 7;
|
| 1265 |
greg |
2.1 |
}
|
| 1266 |
|
|
|
| 1267 |
|
|
/* sky luminance perez model */
|
| 1268 |
greg |
2.9 |
double calc_rel_lum_perez(double dzeta,double gamma,double Z,double epsilon,double Delta,float coeff_perez[])
|
| 1269 |
greg |
2.1 |
{
|
| 1270 |
greg |
2.12 |
|
| 1271 |
greg |
2.1 |
float x[5][4];
|
| 1272 |
|
|
int i,j,num_lin;
|
| 1273 |
|
|
double c_perez[5];
|
| 1274 |
|
|
|
| 1275 |
|
|
if ( (epsilon < skyclearinf) || (epsilon >= skyclearsup) )
|
| 1276 |
|
|
{
|
| 1277 |
greg |
2.14 |
fprintf(stderr,"Error: epsilon out of range in function calc_rel_lum_perez!\n");
|
| 1278 |
greg |
2.1 |
exit(1);
|
| 1279 |
|
|
}
|
| 1280 |
|
|
|
| 1281 |
|
|
/* correction de modele de Perez solar energy ...*/
|
| 1282 |
|
|
if ( (epsilon > 1.065) && (epsilon < 2.8) )
|
| 1283 |
|
|
{
|
| 1284 |
|
|
if ( Delta < 0.2 ) Delta = 0.2;
|
| 1285 |
|
|
}
|
| 1286 |
greg |
2.12 |
|
| 1287 |
|
|
|
| 1288 |
greg |
2.9 |
num_lin = get_numlin(epsilon);
|
| 1289 |
greg |
2.12 |
|
| 1290 |
greg |
2.1 |
for (i=0;i<5;i++)
|
| 1291 |
|
|
for (j=0;j<4;j++)
|
| 1292 |
|
|
{
|
| 1293 |
|
|
x[i][j] = *(coeff_perez + 20*num_lin + 4*i +j);
|
| 1294 |
greg |
2.12 |
/* fprintf(stderr,"x %d %d vaut %f\n",i,j,x[i][j]); */
|
| 1295 |
greg |
2.1 |
}
|
| 1296 |
|
|
|
| 1297 |
|
|
|
| 1298 |
|
|
if (num_lin)
|
| 1299 |
|
|
{
|
| 1300 |
|
|
for (i=0;i<5;i++)
|
| 1301 |
|
|
c_perez[i] = x[i][0] + x[i][1]*Z + Delta * (x[i][2] + x[i][3]*Z);
|
| 1302 |
|
|
}
|
| 1303 |
|
|
else
|
| 1304 |
|
|
{
|
| 1305 |
|
|
c_perez[0] = x[0][0] + x[0][1]*Z + Delta * (x[0][2] + x[0][3]*Z);
|
| 1306 |
|
|
c_perez[1] = x[1][0] + x[1][1]*Z + Delta * (x[1][2] + x[1][3]*Z);
|
| 1307 |
|
|
c_perez[4] = x[4][0] + x[4][1]*Z + Delta * (x[4][2] + x[4][3]*Z);
|
| 1308 |
|
|
c_perez[2] = exp( pow(Delta*(x[2][0]+x[2][1]*Z),x[2][2])) - x[2][3];
|
| 1309 |
|
|
c_perez[3] = -exp( Delta*(x[3][0]+x[3][1]*Z) )+x[3][2]+Delta*x[3][3];
|
| 1310 |
|
|
}
|
| 1311 |
|
|
|
| 1312 |
|
|
|
| 1313 |
|
|
return (1 + c_perez[0]*exp(c_perez[1]/cos(dzeta)) ) *
|
| 1314 |
|
|
(1 + c_perez[2]*exp(c_perez[3]*gamma) +
|
| 1315 |
|
|
c_perez[4]*cos(gamma)*cos(gamma) );
|
| 1316 |
|
|
}
|
| 1317 |
|
|
|
| 1318 |
|
|
|
| 1319 |
|
|
|
| 1320 |
|
|
/* coefficients for the sky luminance perez model */
|
| 1321 |
greg |
2.9 |
void coeff_lum_perez(double Z, double epsilon, double Delta, float coeff_perez[])
|
| 1322 |
greg |
2.1 |
{
|
| 1323 |
|
|
float x[5][4];
|
| 1324 |
|
|
int i,j,num_lin;
|
| 1325 |
|
|
|
| 1326 |
|
|
if ( (epsilon < skyclearinf) || (epsilon >= skyclearsup) )
|
| 1327 |
|
|
{
|
| 1328 |
greg |
2.14 |
fprintf(stderr,"Error: epsilon out of range in function coeff_lum_perez!\n");
|
| 1329 |
greg |
2.1 |
exit(1);
|
| 1330 |
|
|
}
|
| 1331 |
|
|
|
| 1332 |
|
|
/* correction du modele de Perez solar energy ...*/
|
| 1333 |
|
|
if ( (epsilon > 1.065) && (epsilon < 2.8) )
|
| 1334 |
|
|
{
|
| 1335 |
|
|
if ( Delta < 0.2 ) Delta = 0.2;
|
| 1336 |
|
|
}
|
| 1337 |
greg |
2.12 |
|
| 1338 |
|
|
|
| 1339 |
greg |
2.9 |
num_lin = get_numlin(epsilon);
|
| 1340 |
|
|
|
| 1341 |
greg |
2.12 |
/*fprintf(stderr,"numlin %d\n", num_lin);*/
|
| 1342 |
greg |
2.1 |
|
| 1343 |
|
|
for (i=0;i<5;i++)
|
| 1344 |
|
|
for (j=0;j<4;j++)
|
| 1345 |
|
|
{
|
| 1346 |
|
|
x[i][j] = *(coeff_perez + 20*num_lin + 4*i +j);
|
| 1347 |
|
|
/* printf("x %d %d vaut %f\n",i,j,x[i][j]); */
|
| 1348 |
|
|
}
|
| 1349 |
|
|
|
| 1350 |
|
|
|
| 1351 |
|
|
if (num_lin)
|
| 1352 |
|
|
{
|
| 1353 |
|
|
for (i=0;i<5;i++)
|
| 1354 |
|
|
*(c_perez+i) = x[i][0] + x[i][1]*Z + Delta * (x[i][2] + x[i][3]*Z);
|
| 1355 |
|
|
|
| 1356 |
|
|
}
|
| 1357 |
|
|
else
|
| 1358 |
|
|
{
|
| 1359 |
|
|
*(c_perez+0) = x[0][0] + x[0][1]*Z + Delta * (x[0][2] + x[0][3]*Z);
|
| 1360 |
|
|
*(c_perez+1) = x[1][0] + x[1][1]*Z + Delta * (x[1][2] + x[1][3]*Z);
|
| 1361 |
|
|
*(c_perez+4) = x[4][0] + x[4][1]*Z + Delta * (x[4][2] + x[4][3]*Z);
|
| 1362 |
|
|
*(c_perez+2) = exp( pow(Delta*(x[2][0]+x[2][1]*Z),x[2][2])) - x[2][3];
|
| 1363 |
|
|
*(c_perez+3) = -exp( Delta*(x[3][0]+x[3][1]*Z) )+x[3][2]+Delta*x[3][3];
|
| 1364 |
|
|
|
| 1365 |
|
|
|
| 1366 |
|
|
}
|
| 1367 |
|
|
|
| 1368 |
|
|
|
| 1369 |
|
|
return;
|
| 1370 |
|
|
}
|
| 1371 |
|
|
|
| 1372 |
|
|
|
| 1373 |
greg |
2.12 |
|
| 1374 |
greg |
2.1 |
/* degrees into radians */
|
| 1375 |
|
|
double radians(double degres)
|
| 1376 |
|
|
{
|
| 1377 |
greg |
2.9 |
return degres*M_PI/180.0;
|
| 1378 |
greg |
2.1 |
}
|
| 1379 |
|
|
|
| 1380 |
greg |
2.12 |
|
| 1381 |
greg |
2.1 |
/* radian into degrees */
|
| 1382 |
|
|
double degres(double radians)
|
| 1383 |
|
|
{
|
| 1384 |
greg |
2.9 |
return radians/M_PI*180.0;
|
| 1385 |
greg |
2.1 |
}
|
| 1386 |
|
|
|
| 1387 |
greg |
2.12 |
|
| 1388 |
greg |
2.1 |
/* calculation of the angles dzeta and gamma */
|
| 1389 |
|
|
void theta_phi_to_dzeta_gamma(double theta,double phi,double *dzeta,double *gamma, double Z)
|
| 1390 |
|
|
{
|
| 1391 |
|
|
*dzeta = theta; /* dzeta = phi */
|
| 1392 |
|
|
if ( (cos(Z)*cos(theta)+sin(Z)*sin(theta)*cos(phi)) > 1 && (cos(Z)*cos(theta)+sin(Z)*sin(theta)*cos(phi) < 1.1 ) )
|
| 1393 |
|
|
*gamma = 0;
|
| 1394 |
|
|
else if ( (cos(Z)*cos(theta)+sin(Z)*sin(theta)*cos(phi)) > 1.1 )
|
| 1395 |
|
|
{
|
| 1396 |
|
|
printf("error in calculation of gamma (angle between point and sun");
|
| 1397 |
greg |
2.14 |
exit(1);
|
| 1398 |
greg |
2.1 |
}
|
| 1399 |
|
|
else
|
| 1400 |
|
|
*gamma = acos(cos(Z)*cos(theta)+sin(Z)*sin(theta)*cos(phi));
|
| 1401 |
|
|
}
|
| 1402 |
|
|
|
| 1403 |
|
|
|
| 1404 |
|
|
|
| 1405 |
|
|
double integ_lv(float *lv,float *theta)
|
| 1406 |
|
|
{
|
| 1407 |
|
|
int i;
|
| 1408 |
|
|
double buffer=0.0;
|
| 1409 |
greg |
2.12 |
|
| 1410 |
greg |
2.1 |
for (i=0;i<145;i++)
|
| 1411 |
greg |
2.12 |
{
|
| 1412 |
greg |
2.1 |
buffer += (*(lv+i))*cos(radians(*(theta+i)));
|
| 1413 |
greg |
2.12 |
}
|
| 1414 |
|
|
|
| 1415 |
greg |
2.9 |
return buffer*2*M_PI/144;
|
| 1416 |
greg |
2.1 |
}
|
| 1417 |
|
|
|
| 1418 |
|
|
|
| 1419 |
|
|
|
| 1420 |
|
|
/* enter day number(double), return E0 = square(R0/R): eccentricity correction factor */
|
| 1421 |
|
|
|
| 1422 |
|
|
double get_eccentricity()
|
| 1423 |
|
|
{
|
| 1424 |
|
|
double day_angle;
|
| 1425 |
|
|
double E0;
|
| 1426 |
|
|
|
| 1427 |
greg |
2.9 |
day_angle = 2*M_PI*(daynumber - 1)/365;
|
| 1428 |
greg |
2.1 |
E0 = 1.00011+0.034221*cos(day_angle)+0.00128*sin(day_angle)+
|
| 1429 |
|
|
0.000719*cos(2*day_angle)+0.000077*sin(2*day_angle);
|
| 1430 |
|
|
|
| 1431 |
|
|
return (E0);
|
| 1432 |
|
|
}
|
| 1433 |
|
|
|
| 1434 |
|
|
|
| 1435 |
|
|
/* enter sunzenith angle (degrees) return relative air mass (double) */
|
| 1436 |
|
|
double air_mass()
|
| 1437 |
|
|
{
|
| 1438 |
|
|
double m;
|
| 1439 |
|
|
if (sunzenith>90)
|
| 1440 |
|
|
{
|
| 1441 |
greg |
2.14 |
if(suppress_warnings==0)
|
| 1442 |
|
|
{ fprintf(stderr, "Warning: air mass has reached the maximal value\n"); }
|
| 1443 |
|
|
sunzenith=90;
|
| 1444 |
greg |
2.1 |
}
|
| 1445 |
greg |
2.9 |
m = 1/( cos(sunzenith*M_PI/180)+0.15*exp( log(93.885-sunzenith)*(-1.253) ) );
|
| 1446 |
greg |
2.1 |
return(m);
|
| 1447 |
|
|
}
|
| 1448 |
|
|
|
| 1449 |
|
|
|
| 1450 |
|
|
|