/* * 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 #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); }