/*
* Copyright (c) 1993, 1999 Alexandre Wennmacher (wennmach@geo.Uni-Koeln.DE)
* All rights reserved.
*
* Redistribution and use in source and binary forms, with or without
* modification, are permitted provided that the following conditions
* are met:
* 1. Redistributions of source code must retain the above copyright
* notice, this list of conditions and the following disclaimer.
* 2. Redistributions in binary form must reproduce the above copyright
* notice, this list of conditions and the following disclaimer in the
* documentation and/or other materials provided with the distribution.
* 3. All advertising materials mentioning features or use of this software
* must display the following acknowledgement:
* This product includes software developed by Alexandre Wennmacher.
* 4. The name of Alexandre Wennmacher may not be used to endorse or promote
* products derived from this software without specific prior written
* permission.
*
* THIS SOFTWARE IS PROVIDED BY ALEXANDRE WENNMACHER AND CONTRIBUTORS ``AS IS''
* AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
* IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
* ARE DISCLAIMED. IN NO EVENT SHALL ALEXANDRE WENNMACHER OR CONTRIBUTORS BE
* LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR
* CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF
* SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS
* INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN
* CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)
* ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
* POSSIBILITY OF SUCH DAMAGE.
*
*/
#include <math.h>
#include "const.h"
double
EqunofTime(double JulianDate, double *SunRa, double *SunDec)
{
double n, L, g, lambda, epsilon;
n = JulianDate - 2451545.0;
L = 280.460 + 0.9856474*n;
g = 357.528 + 0.9856003*n;
while (L < 0.0) L += 360.0;
while (L >= 360.0) L -= 360.0;
while (g < 0.0) g += 360.0;
while (g > 360.0) g -= 360.0;
lambda = L + 1.915*sin(DEGTORAD*g) + 0.020*sin(2.0*DEGTORAD*g);
epsilon = 23.439 - 0.0000004*n;
*SunRa = atan(cos(DEGTORAD*epsilon)*tan(DEGTORAD*lambda));
*SunDec = asin(sin(DEGTORAD*epsilon)*sin(DEGTORAD*lambda));
if (*SunRa < 0.0) *SunRa += TWO_PI;
lambda *= DEGTORAD;
while (sin(lambda)*sin(*SunRa) < 0.0 || cos(lambda)*cos(*SunRa) < 0.0) {
*SunRa += PI_2;
if (*SunRa >= TWO_PI) *SunRa -= TWO_PI;
}
return(DEGTORAD*L - *SunRa);
}
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