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view on githubraw file Latest commit 27f9df09 on 2018-02-19 15:43:37 UTC27f9df093b Oliv*0001 #include "SUN_OPTIONS.h" 0002 0003 CBOP 0004 C !ROUTINE: SUN_NUTATE 0005 0006 C !INTERFACE: ====================================================== 0007 SUBROUTINE SUN_NUTATE( 0008 I t, xls, gs, xlm, asc, 0009 O dpsi, eps ) 0010 0011 C !DESCRIPTION: 0012 C This subroutine computes the nutation in longitude and the obliquity 0013 C of the ecliptic corrected for nutation. It uses the model referenced 0014 C in The Astronomical Almanac for 1984, Section S (Supplement) and 0015 C documented in Exact closed-form geolocation algorithm for Earth 0016 C survey sensors, by F.S. Patt and W.W. Gregg, Int. Journal of 0017 C Remote Sensing, 1993. These parameters are used to compute the 0018 C apparent time correction to the Greenwich Hour Angle and for the 0019 C calculation of the geocentric Sun vector. The input ephemeris 0020 C parameters are computed using subroutine ephparms. Terms are 0021 C included to 0.1 arcsecond. 0022 C 0023 C Program written by: Frederick S. Patt 0024 C General Sciences Corporation 0025 C October 21, 1992 0026 0027 C !USES: =========================================================== 0028 IMPLICIT NONE 0029 #include "SIZE.h" 0030 #include "EEPARAMS.h" 0031 #include "PARAMS.h" 0032 0033 C !INPUT PARAMETERS: =============================================== 0034 C t :: Time in days since January 1, 2000 at 12 hours UT 0035 C xls :: Mean solar longitude (degrees) 0036 C gs :: Mean solar anomaly (degrees) 0037 C xlm :: Mean lunar longitude (degrees) 0038 C asc :: Ascending node of mean lunar orbit 0039 _RL t, xls, gs, xlm, asc 0040 0041 C !OUTPUT PARAMETERS: ============================================== 0042 C dPsi :: Nutation in longitude (degrees) 0043 C Eps :: Obliquity of the Ecliptic (degrees) 0044 C (includes nutation in obliquity) 0045 _RL dpsi, eps 0046 CEOP 0047 0048 #ifdef ALLOW_SUN 0049 0050 C !LOCAL VARIABLES: ================================================ 0051 _RL epsm, deps 0052 0053 C Nutation in Longitude 0054 dpsi = - 17.1996 _d 0*SIN(asc*deg2rad) 0055 & + 0.2062 _d 0*SIN(2.0 _d 0*asc*deg2rad) 0056 & - 1.3187 _d 0*SIN(2.0 _d 0*xls*deg2rad) 0057 & + 0.1426 _d 0*SIN(gs*deg2rad) 0058 & - 0.2274 _d 0*SIN(2.0 _d 0*xlm*deg2rad) 0059 0060 C Mean Obliquity of the Ecliptic 0061 epsm = 23.439291 _d 0 - 3.560 _d -7*t 0062 0063 C Nutation in Obliquity 0064 deps = 9.2025 _d 0*COS(asc*deg2rad) + 0065 & 0.5736 _d 0*COS(2.0 _d 0*xls*deg2rad) 0066 0067 C True Obliquity of the Ecliptic 0068 eps = epsm + deps/3600.0 _d 0 0069 0070 dpsi = dpsi/3600.0 _d 0 0071 0072 #endif 0073 0074 RETURN 0075 END
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