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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/slalib/nutc80.f | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/nutc80.f')
-rw-r--r-- | math/slalib/nutc80.f | 476 |
1 files changed, 476 insertions, 0 deletions
diff --git a/math/slalib/nutc80.f b/math/slalib/nutc80.f new file mode 100644 index 00000000..4d27e331 --- /dev/null +++ b/math/slalib/nutc80.f @@ -0,0 +1,476 @@ + SUBROUTINE slNUTC80 (DATE, DPSI, DEPS, EPS0) +*+ +* - - - - - - - +* N U T C 8 0 +* - - - - - - - +* +* Nutation: longitude & obliquity components and mean obliquity, +* using the IAU 1980 theory (double precision) +* +* Given: +* DATE d TDB (loosely ET) as Modified Julian Date +* (JD-2400000.5) +* Returned: +* DPSI,DEPS d nutation in longitude,obliquity +* EPS0 d mean obliquity +* +* Called: slDA1P +* +* Notes: +* +* 1 Earth attitude predictions made by combining the present nutation +* model with IAU 1976 precession are accurate to 0.35 arcsec over +* the interval 1900-2100. (The accuracy is much better near the +* middle of the interval.) +* +* 2 The slNUTC routine is the equivalent of the present routine +* but using the Shirai & Fukushima 2001 forced nutation theory +* (SF2001). The newer theory is more accurate than IAU 1980, +* within 1 mas (with respect to the ICRF) for a few decades around +* 2000. The improvement is mainly because of the corrections to the +* IAU 1976 precession that the SF2001 theory includes. +* +* References: +* Final report of the IAU Working Group on Nutation, +* chairman P.K.Seidelmann, 1980. +* Kaplan,G.H., 1981, USNO circular no. 163, pA3-6. +* +* P.T.Wallace Starlink 7 October 2001 +* +* Copyright (C) 2001 Rutherford Appleton Laboratory +* +* License: +* This program is free software; you can redistribute it and/or modify +* it under the terms of the GNU General Public License as published by +* the Free Software Foundation; either version 2 of the License, or +* (at your option) any later version. +* +* This program is distributed in the hope that it will be useful, +* but WITHOUT ANY WARRANTY; without even the implied warranty of +* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the +* GNU General Public License for more details. +* +* You should have received a copy of the GNU General Public License +* along with this program (see SLA_CONDITIONS); if not, write to the +* Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor, +* Boston, MA 02110-1301 USA +* +* Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. +*- + + IMPLICIT NONE + + DOUBLE PRECISION DATE,DPSI,DEPS,EPS0 + + DOUBLE PRECISION T2AS,AS2R,U2R + DOUBLE PRECISION T,EL,EL2,EL3 + DOUBLE PRECISION ELP,ELP2 + DOUBLE PRECISION F,F2,F4 + DOUBLE PRECISION D,D2,D4 + DOUBLE PRECISION OM,OM2 + DOUBLE PRECISION DP,DE + DOUBLE PRECISION A + + DOUBLE PRECISION slDA1P + + +* Turns to arc seconds + PARAMETER (T2AS=1296000D0) +* Arc seconds to radians + PARAMETER (AS2R=0.484813681109535994D-5) +* Units of 0.0001 arcsec to radians + PARAMETER (U2R=AS2R/1D4) + + + + +* Interval between basic epoch J2000.0 and current epoch (JC) + T=(DATE-51544.5D0)/36525D0 + +* +* FUNDAMENTAL ARGUMENTS in the FK5 reference system +* + +* Mean longitude of the Moon minus mean longitude of the Moon's perigee + EL=slDA1P(AS2R*(485866.733D0+(1325D0*T2AS+715922.633D0 + : +(31.310D0+0.064D0*T)*T)*T)) + +* Mean longitude of the Sun minus mean longitude of the Sun's perigee + ELP=slDA1P(AS2R*(1287099.804D0+(99D0*T2AS+1292581.224D0 + : +(-0.577D0-0.012D0*T)*T)*T)) + +* Mean longitude of the Moon minus mean longitude of the Moon's node + F=slDA1P(AS2R*(335778.877D0+(1342D0*T2AS+295263.137D0 + : +(-13.257D0+0.011D0*T)*T)*T)) + +* Mean elongation of the Moon from the Sun + D=slDA1P(AS2R*(1072261.307D0+(1236D0*T2AS+1105601.328D0 + : +(-6.891D0+0.019D0*T)*T)*T)) + +* Longitude of the mean ascending node of the lunar orbit on the +* ecliptic, measured from the mean equinox of date + OM=slDA1P(AS2R*(450160.280D0+(-5D0*T2AS-482890.539D0 + : +(7.455D0+0.008D0*T)*T)*T)) + +* Multiples of arguments + EL2=EL+EL + EL3=EL2+EL + ELP2=ELP+ELP + F2=F+F + F4=F2+F2 + D2=D+D + D4=D2+D2 + OM2=OM+OM + + +* +* SERIES FOR THE NUTATION +* + DP=0D0 + DE=0D0 + +* 106 + DP=DP+SIN(ELP+D) +* 105 + DP=DP-SIN(F2+D4+OM2) +* 104 + DP=DP+SIN(EL2+D2) +* 103 + DP=DP-SIN(EL-F2+D2) +* 102 + DP=DP-SIN(EL+ELP-D2+OM) +* 101 + DP=DP-SIN(-ELP+F2+OM) +* 100 + DP=DP-SIN(EL-F2-D2) +* 99 + DP=DP-SIN(ELP+D2) +* 98 + DP=DP-SIN(F2-D+OM2) +* 97 + DP=DP-SIN(-F2+OM) +* 96 + DP=DP+SIN(-EL-ELP+D2+OM) +* 95 + DP=DP+SIN(ELP+F2+OM) +* 94 + DP=DP-SIN(EL+F2-D2) +* 93 + DP=DP+SIN(EL3+F2-D2+OM2) +* 92 + DP=DP+SIN(F4-D2+OM2) +* 91 + DP=DP-SIN(EL+D2+OM) +* 90 + DP=DP-SIN(EL2+F2+D2+OM2) +* 89 + A=EL2+F2-D2+OM + DP=DP+SIN(A) + DE=DE-COS(A) +* 88 + DP=DP+SIN(EL-ELP-D2) +* 87 + DP=DP+SIN(-EL+F4+OM2) +* 86 + A=-EL2+F2+D4+OM2 + DP=DP-SIN(A) + DE=DE+COS(A) +* 85 + A=EL+F2+D2+OM + DP=DP-SIN(A) + DE=DE+COS(A) +* 84 + A=EL+ELP+F2-D2+OM2 + DP=DP+SIN(A) + DE=DE-COS(A) +* 83 + DP=DP-SIN(EL2-D4) +* 82 + A=-EL+F2+D4+OM2 + DP=DP-2D0*SIN(A) + DE=DE+COS(A) +* 81 + A=-EL2+F2+D2+OM2 + DP=DP+SIN(A) + DE=DE-COS(A) +* 80 + DP=DP-SIN(EL-D4) +* 79 + A=-EL+OM2 + DP=DP+SIN(A) + DE=DE-COS(A) +* 78 + A=F2+D+OM2 + DP=DP+2D0*SIN(A) + DE=DE-COS(A) +* 77 + DP=DP+2D0*SIN(EL3) +* 76 + A=EL+OM2 + DP=DP-2D0*SIN(A) + DE=DE+COS(A) +* 75 + A=EL2+OM + DP=DP+2D0*SIN(A) + DE=DE-COS(A) +* 74 + A=-EL+F2-D2+OM + DP=DP-2D0*SIN(A) + DE=DE+COS(A) +* 73 + A=EL+ELP+F2+OM2 + DP=DP+2D0*SIN(A) + DE=DE-COS(A) +* 72 + A=-ELP+F2+D2+OM2 + DP=DP-3D0*SIN(A) + DE=DE+COS(A) +* 71 + A=EL3+F2+OM2 + DP=DP-3D0*SIN(A) + DE=DE+COS(A) +* 70 + A=-EL2+OM + DP=DP-2D0*SIN(A) + DE=DE+COS(A) +* 69 + A=-EL-ELP+F2+D2+OM2 + DP=DP-3D0*SIN(A) + DE=DE+COS(A) +* 68 + A=EL-ELP+F2+OM2 + DP=DP-3D0*SIN(A) + DE=DE+COS(A) +* 67 + DP=DP+3D0*SIN(EL+F2) +* 66 + DP=DP-3D0*SIN(EL+ELP) +* 65 + DP=DP-4D0*SIN(D) +* 64 + DP=DP+4D0*SIN(EL-F2) +* 63 + DP=DP-4D0*SIN(ELP-D2) +* 62 + A=EL2+F2+OM + DP=DP-5D0*SIN(A) + DE=DE+3D0*COS(A) +* 61 + DP=DP+5D0*SIN(EL-ELP) +* 60 + A=-D2+OM + DP=DP-5D0*SIN(A) + DE=DE+3D0*COS(A) +* 59 + A=EL+F2-D2+OM + DP=DP+6D0*SIN(A) + DE=DE-3D0*COS(A) +* 58 + A=F2+D2+OM + DP=DP-7D0*SIN(A) + DE=DE+3D0*COS(A) +* 57 + A=D2+OM + DP=DP-6D0*SIN(A) + DE=DE+3D0*COS(A) +* 56 + A=EL2+F2-D2+OM2 + DP=DP+6D0*SIN(A) + DE=DE-3D0*COS(A) +* 55 + DP=DP+6D0*SIN(EL+D2) +* 54 + A=EL+F2+D2+OM2 + DP=DP-8D0*SIN(A) + DE=DE+3D0*COS(A) +* 53 + A=-ELP+F2+OM2 + DP=DP-7D0*SIN(A) + DE=DE+3D0*COS(A) +* 52 + A=ELP+F2+OM2 + DP=DP+7D0*SIN(A) + DE=DE-3D0*COS(A) +* 51 + DP=DP-7D0*SIN(EL+ELP-D2) +* 50 + A=-EL+F2+D2+OM + DP=DP-10D0*SIN(A) + DE=DE+5D0*COS(A) +* 49 + A=EL-D2+OM + DP=DP-13D0*SIN(A) + DE=DE+7D0*COS(A) +* 48 + A=-EL+D2+OM + DP=DP+16D0*SIN(A) + DE=DE-8D0*COS(A) +* 47 + A=-EL+F2+OM + DP=DP+21D0*SIN(A) + DE=DE-10D0*COS(A) +* 46 + DP=DP+26D0*SIN(F2) + DE=DE-COS(F2) +* 45 + A=EL2+F2+OM2 + DP=DP-31D0*SIN(A) + DE=DE+13D0*COS(A) +* 44 + A=EL+F2-D2+OM2 + DP=DP+29D0*SIN(A) + DE=DE-12D0*COS(A) +* 43 + DP=DP+29D0*SIN(EL2) + DE=DE-COS(EL2) +* 42 + A=F2+D2+OM2 + DP=DP-38D0*SIN(A) + DE=DE+16D0*COS(A) +* 41 + A=EL+F2+OM + DP=DP-51D0*SIN(A) + DE=DE+27D0*COS(A) +* 40 + A=-EL+F2+D2+OM2 + DP=DP-59D0*SIN(A) + DE=DE+26D0*COS(A) +* 39 + A=-EL+OM + DP=DP+(-58D0-0.1D0*T)*SIN(A) + DE=DE+32D0*COS(A) +* 38 + A=EL+OM + DP=DP+(63D0+0.1D0*T)*SIN(A) + DE=DE-33D0*COS(A) +* 37 + DP=DP+63D0*SIN(D2) + DE=DE-2D0*COS(D2) +* 36 + A=-EL+F2+OM2 + DP=DP+123D0*SIN(A) + DE=DE-53D0*COS(A) +* 35 + A=EL-D2 + DP=DP-158D0*SIN(A) + DE=DE-COS(A) +* 34 + A=EL+F2+OM2 + DP=DP-301D0*SIN(A) + DE=DE+(129D0-0.1D0*T)*COS(A) +* 33 + A=F2+OM + DP=DP+(-386D0-0.4D0*T)*SIN(A) + DE=DE+200D0*COS(A) +* 32 + DP=DP+(712D0+0.1D0*T)*SIN(EL) + DE=DE-7D0*COS(EL) +* 31 + A=F2+OM2 + DP=DP+(-2274D0-0.2D0*T)*SIN(A) + DE=DE+(977D0-0.5D0*T)*COS(A) +* 30 + DP=DP-SIN(ELP+F2-D2) +* 29 + DP=DP+SIN(-EL+D+OM) +* 28 + DP=DP+SIN(ELP+OM2) +* 27 + DP=DP-SIN(ELP-F2+D2) +* 26 + DP=DP+SIN(-F2+D2+OM) +* 25 + DP=DP+SIN(EL2+ELP-D2) +* 24 + DP=DP-4D0*SIN(EL-D) +* 23 + A=ELP+F2-D2+OM + DP=DP+4D0*SIN(A) + DE=DE-2D0*COS(A) +* 22 + A=EL2-D2+OM + DP=DP+4D0*SIN(A) + DE=DE-2D0*COS(A) +* 21 + A=-ELP+F2-D2+OM + DP=DP-5D0*SIN(A) + DE=DE+3D0*COS(A) +* 20 + A=-EL2+D2+OM + DP=DP-6D0*SIN(A) + DE=DE+3D0*COS(A) +* 19 + A=-ELP+OM + DP=DP-12D0*SIN(A) + DE=DE+6D0*COS(A) +* 18 + A=ELP2+F2-D2+OM2 + DP=DP+(-16D0+0.1D0*T)*SIN(A) + DE=DE+7D0*COS(A) +* 17 + A=ELP+OM + DP=DP-15D0*SIN(A) + DE=DE+9D0*COS(A) +* 16 + DP=DP+(17D0-0.1D0*T)*SIN(ELP2) +* 15 + DP=DP-22D0*SIN(F2-D2) +* 14 + A=EL2-D2 + DP=DP+48D0*SIN(A) + DE=DE+COS(A) +* 13 + A=F2-D2+OM + DP=DP+(129D0+0.1D0*T)*SIN(A) + DE=DE-70D0*COS(A) +* 12 + A=-ELP+F2-D2+OM2 + DP=DP+(217D0-0.5D0*T)*SIN(A) + DE=DE+(-95D0+0.3D0*T)*COS(A) +* 11 + A=ELP+F2-D2+OM2 + DP=DP+(-517D0+1.2D0*T)*SIN(A) + DE=DE+(224D0-0.6D0*T)*COS(A) +* 10 + DP=DP+(1426D0-3.4D0*T)*SIN(ELP) + DE=DE+(54D0-0.1D0*T)*COS(ELP) +* 9 + A=F2-D2+OM2 + DP=DP+(-13187D0-1.6D0*T)*SIN(A) + DE=DE+(5736D0-3.1D0*T)*COS(A) +* 8 + DP=DP+SIN(EL2-F2+OM) +* 7 + A=-ELP2+F2-D2+OM + DP=DP-2D0*SIN(A) + DE=DE+1D0*COS(A) +* 6 + DP=DP-3D0*SIN(EL-ELP-D) +* 5 + A=-EL2+F2+OM2 + DP=DP-3D0*SIN(A) + DE=DE+1D0*COS(A) +* 4 + DP=DP+11D0*SIN(EL2-F2) +* 3 + A=-EL2+F2+OM + DP=DP+46D0*SIN(A) + DE=DE-24D0*COS(A) +* 2 + DP=DP+(2062D0+0.2D0*T)*SIN(OM2) + DE=DE+(-895D0+0.5D0*T)*COS(OM2) +* 1 + DP=DP+(-171996D0-174.2D0*T)*SIN(OM) + DE=DE+(92025D0+8.9D0*T)*COS(OM) + +* Convert results to radians + DPSI=DP*U2R + DEPS=DE*U2R + +* Mean obliquity + EPS0=AS2R*(84381.448D0+ + : (-46.8150D0+ + : (-0.00059D0+ + : 0.001813D0*T)*T)*T) + + END |