line |
stmt |
bran |
cond |
sub |
pod |
time |
code |
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#include "erfa.h" |
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void eraNut80(double date1, double date2, double *dpsi, double *deps) |
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/* |
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** - - - - - - - - - |
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** e r a N u t 8 0 |
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** - - - - - - - - - |
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** |
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** Nutation, IAU 1980 model. |
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** |
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** Given: |
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** date1,date2 double TT as a 2-part Julian Date (Note 1) |
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** |
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** Returned: |
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** dpsi double nutation in longitude (radians) |
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** deps double nutation in obliquity (radians) |
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** |
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** Notes: |
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** |
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** 1) The TT date date1+date2 is a Julian Date, apportioned in any |
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** convenient way between the two arguments. For example, |
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** JD(TT)=2450123.7 could be expressed in any of these ways, |
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** among others: |
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** |
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** date1 date2 |
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** |
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** 2450123.7 0.0 (JD method) |
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** 2451545.0 -1421.3 (J2000 method) |
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** 2400000.5 50123.2 (MJD method) |
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** 2450123.5 0.2 (date & time method) |
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** |
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** The JD method is the most natural and convenient to use in |
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** cases where the loss of several decimal digits of resolution |
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** is acceptable. The J2000 method is best matched to the way |
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** the argument is handled internally and will deliver the |
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** optimum resolution. The MJD method and the date & time methods |
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** are both good compromises between resolution and convenience. |
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** |
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** 2) The nutation components are with respect to the ecliptic of |
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** date. |
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** |
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** Called: |
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** eraAnpm normalize angle into range +/- pi |
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** |
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** Reference: |
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** |
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** Explanatory Supplement to the Astronomical Almanac, |
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** P. Kenneth Seidelmann (ed), University Science Books (1992), |
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** Section 3.222 (p111). |
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** |
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** Copyright (C) 2013-2020, NumFOCUS Foundation. |
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** Derived, with permission, from the SOFA library. See notes at end of file. |
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*/ |
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{ |
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double t, el, elp, f, d, om, dp, de, arg, s, c; |
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int j; |
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58
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/* Units of 0.1 milliarcsecond to radians */ |
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const double U2R = ERFA_DAS2R / 1e4; |
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61
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/* ------------------------------------------------ */ |
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/* Table of multiples of arguments and coefficients */ |
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/* ------------------------------------------------ */ |
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65
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/* The units for the sine and cosine coefficients are 0.1 mas and */ |
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/* the same per Julian century */ |
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static const struct { |
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int nl,nlp,nf,nd,nom; /* coefficients of l,l',F,D,Om */ |
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double sp,spt; /* longitude sine, 1 and t coefficients */ |
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double ce,cet; /* obliquity cosine, 1 and t coefficients */ |
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} x[] = { |
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74
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/* 1-10 */ |
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{ 0, 0, 0, 0, 1, -171996.0, -174.2, 92025.0, 8.9 }, |
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{ 0, 0, 0, 0, 2, 2062.0, 0.2, -895.0, 0.5 }, |
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{ -2, 0, 2, 0, 1, 46.0, 0.0, -24.0, 0.0 }, |
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{ 2, 0, -2, 0, 0, 11.0, 0.0, 0.0, 0.0 }, |
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{ -2, 0, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 }, |
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{ 1, -1, 0, -1, 0, -3.0, 0.0, 0.0, 0.0 }, |
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{ 0, -2, 2, -2, 1, -2.0, 0.0, 1.0, 0.0 }, |
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{ 2, 0, -2, 0, 1, 1.0, 0.0, 0.0, 0.0 }, |
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{ 0, 0, 2, -2, 2, -13187.0, -1.6, 5736.0, -3.1 }, |
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{ 0, 1, 0, 0, 0, 1426.0, -3.4, 54.0, -0.1 }, |
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/* 11-20 */ |
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{ 0, 1, 2, -2, 2, -517.0, 1.2, 224.0, -0.6 }, |
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{ 0, -1, 2, -2, 2, 217.0, -0.5, -95.0, 0.3 }, |
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{ 0, 0, 2, -2, 1, 129.0, 0.1, -70.0, 0.0 }, |
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{ 2, 0, 0, -2, 0, 48.0, 0.0, 1.0, 0.0 }, |
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{ 0, 0, 2, -2, 0, -22.0, 0.0, 0.0, 0.0 }, |
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{ 0, 2, 0, 0, 0, 17.0, -0.1, 0.0, 0.0 }, |
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{ 0, 1, 0, 0, 1, -15.0, 0.0, 9.0, 0.0 }, |
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{ 0, 2, 2, -2, 2, -16.0, 0.1, 7.0, 0.0 }, |
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{ 0, -1, 0, 0, 1, -12.0, 0.0, 6.0, 0.0 }, |
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{ -2, 0, 0, 2, 1, -6.0, 0.0, 3.0, 0.0 }, |
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/* 21-30 */ |
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{ 0, -1, 2, -2, 1, -5.0, 0.0, 3.0, 0.0 }, |
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{ 2, 0, 0, -2, 1, 4.0, 0.0, -2.0, 0.0 }, |
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{ 0, 1, 2, -2, 1, 4.0, 0.0, -2.0, 0.0 }, |
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{ 1, 0, 0, -1, 0, -4.0, 0.0, 0.0, 0.0 }, |
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{ 2, 1, 0, -2, 0, 1.0, 0.0, 0.0, 0.0 }, |
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{ 0, 0, -2, 2, 1, 1.0, 0.0, 0.0, 0.0 }, |
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{ 0, 1, -2, 2, 0, -1.0, 0.0, 0.0, 0.0 }, |
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{ 0, 1, 0, 0, 2, 1.0, 0.0, 0.0, 0.0 }, |
107
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{ -1, 0, 0, 1, 1, 1.0, 0.0, 0.0, 0.0 }, |
108
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{ 0, 1, 2, -2, 0, -1.0, 0.0, 0.0, 0.0 }, |
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110
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/* 31-40 */ |
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{ 0, 0, 2, 0, 2, -2274.0, -0.2, 977.0, -0.5 }, |
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{ 1, 0, 0, 0, 0, 712.0, 0.1, -7.0, 0.0 }, |
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{ 0, 0, 2, 0, 1, -386.0, -0.4, 200.0, 0.0 }, |
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{ 1, 0, 2, 0, 2, -301.0, 0.0, 129.0, -0.1 }, |
115
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{ 1, 0, 0, -2, 0, -158.0, 0.0, -1.0, 0.0 }, |
116
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{ -1, 0, 2, 0, 2, 123.0, 0.0, -53.0, 0.0 }, |
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{ 0, 0, 0, 2, 0, 63.0, 0.0, -2.0, 0.0 }, |
118
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{ 1, 0, 0, 0, 1, 63.0, 0.1, -33.0, 0.0 }, |
119
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{ -1, 0, 0, 0, 1, -58.0, -0.1, 32.0, 0.0 }, |
120
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{ -1, 0, 2, 2, 2, -59.0, 0.0, 26.0, 0.0 }, |
121
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122
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/* 41-50 */ |
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{ 1, 0, 2, 0, 1, -51.0, 0.0, 27.0, 0.0 }, |
124
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{ 0, 0, 2, 2, 2, -38.0, 0.0, 16.0, 0.0 }, |
125
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{ 2, 0, 0, 0, 0, 29.0, 0.0, -1.0, 0.0 }, |
126
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{ 1, 0, 2, -2, 2, 29.0, 0.0, -12.0, 0.0 }, |
127
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{ 2, 0, 2, 0, 2, -31.0, 0.0, 13.0, 0.0 }, |
128
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{ 0, 0, 2, 0, 0, 26.0, 0.0, -1.0, 0.0 }, |
129
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{ -1, 0, 2, 0, 1, 21.0, 0.0, -10.0, 0.0 }, |
130
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{ -1, 0, 0, 2, 1, 16.0, 0.0, -8.0, 0.0 }, |
131
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{ 1, 0, 0, -2, 1, -13.0, 0.0, 7.0, 0.0 }, |
132
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{ -1, 0, 2, 2, 1, -10.0, 0.0, 5.0, 0.0 }, |
133
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134
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/* 51-60 */ |
135
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{ 1, 1, 0, -2, 0, -7.0, 0.0, 0.0, 0.0 }, |
136
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{ 0, 1, 2, 0, 2, 7.0, 0.0, -3.0, 0.0 }, |
137
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{ 0, -1, 2, 0, 2, -7.0, 0.0, 3.0, 0.0 }, |
138
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{ 1, 0, 2, 2, 2, -8.0, 0.0, 3.0, 0.0 }, |
139
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{ 1, 0, 0, 2, 0, 6.0, 0.0, 0.0, 0.0 }, |
140
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{ 2, 0, 2, -2, 2, 6.0, 0.0, -3.0, 0.0 }, |
141
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{ 0, 0, 0, 2, 1, -6.0, 0.0, 3.0, 0.0 }, |
142
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{ 0, 0, 2, 2, 1, -7.0, 0.0, 3.0, 0.0 }, |
143
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{ 1, 0, 2, -2, 1, 6.0, 0.0, -3.0, 0.0 }, |
144
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{ 0, 0, 0, -2, 1, -5.0, 0.0, 3.0, 0.0 }, |
145
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146
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/* 61-70 */ |
147
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{ 1, -1, 0, 0, 0, 5.0, 0.0, 0.0, 0.0 }, |
148
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{ 2, 0, 2, 0, 1, -5.0, 0.0, 3.0, 0.0 }, |
149
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{ 0, 1, 0, -2, 0, -4.0, 0.0, 0.0, 0.0 }, |
150
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{ 1, 0, -2, 0, 0, 4.0, 0.0, 0.0, 0.0 }, |
151
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{ 0, 0, 0, 1, 0, -4.0, 0.0, 0.0, 0.0 }, |
152
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{ 1, 1, 0, 0, 0, -3.0, 0.0, 0.0, 0.0 }, |
153
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{ 1, 0, 2, 0, 0, 3.0, 0.0, 0.0, 0.0 }, |
154
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{ 1, -1, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 }, |
155
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{ -1, -1, 2, 2, 2, -3.0, 0.0, 1.0, 0.0 }, |
156
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{ -2, 0, 0, 0, 1, -2.0, 0.0, 1.0, 0.0 }, |
157
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158
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/* 71-80 */ |
159
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{ 3, 0, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 }, |
160
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{ 0, -1, 2, 2, 2, -3.0, 0.0, 1.0, 0.0 }, |
161
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{ 1, 1, 2, 0, 2, 2.0, 0.0, -1.0, 0.0 }, |
162
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{ -1, 0, 2, -2, 1, -2.0, 0.0, 1.0, 0.0 }, |
163
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{ 2, 0, 0, 0, 1, 2.0, 0.0, -1.0, 0.0 }, |
164
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{ 1, 0, 0, 0, 2, -2.0, 0.0, 1.0, 0.0 }, |
165
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{ 3, 0, 0, 0, 0, 2.0, 0.0, 0.0, 0.0 }, |
166
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{ 0, 0, 2, 1, 2, 2.0, 0.0, -1.0, 0.0 }, |
167
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{ -1, 0, 0, 0, 2, 1.0, 0.0, -1.0, 0.0 }, |
168
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{ 1, 0, 0, -4, 0, -1.0, 0.0, 0.0, 0.0 }, |
169
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170
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/* 81-90 */ |
171
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{ -2, 0, 2, 2, 2, 1.0, 0.0, -1.0, 0.0 }, |
172
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{ -1, 0, 2, 4, 2, -2.0, 0.0, 1.0, 0.0 }, |
173
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{ 2, 0, 0, -4, 0, -1.0, 0.0, 0.0, 0.0 }, |
174
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{ 1, 1, 2, -2, 2, 1.0, 0.0, -1.0, 0.0 }, |
175
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{ 1, 0, 2, 2, 1, -1.0, 0.0, 1.0, 0.0 }, |
176
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{ -2, 0, 2, 4, 2, -1.0, 0.0, 1.0, 0.0 }, |
177
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{ -1, 0, 4, 0, 2, 1.0, 0.0, 0.0, 0.0 }, |
178
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{ 1, -1, 0, -2, 0, 1.0, 0.0, 0.0, 0.0 }, |
179
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{ 2, 0, 2, -2, 1, 1.0, 0.0, -1.0, 0.0 }, |
180
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{ 2, 0, 2, 2, 2, -1.0, 0.0, 0.0, 0.0 }, |
181
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182
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/* 91-100 */ |
183
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{ 1, 0, 0, 2, 1, -1.0, 0.0, 0.0, 0.0 }, |
184
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{ 0, 0, 4, -2, 2, 1.0, 0.0, 0.0, 0.0 }, |
185
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{ 3, 0, 2, -2, 2, 1.0, 0.0, 0.0, 0.0 }, |
186
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{ 1, 0, 2, -2, 0, -1.0, 0.0, 0.0, 0.0 }, |
187
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{ 0, 1, 2, 0, 1, 1.0, 0.0, 0.0, 0.0 }, |
188
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{ -1, -1, 0, 2, 1, 1.0, 0.0, 0.0, 0.0 }, |
189
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{ 0, 0, -2, 0, 1, -1.0, 0.0, 0.0, 0.0 }, |
190
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{ 0, 0, 2, -1, 2, -1.0, 0.0, 0.0, 0.0 }, |
191
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{ 0, 1, 0, 2, 0, -1.0, 0.0, 0.0, 0.0 }, |
192
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{ 1, 0, -2, -2, 0, -1.0, 0.0, 0.0, 0.0 }, |
193
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194
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/* 101-106 */ |
195
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{ 0, -1, 2, 0, 1, -1.0, 0.0, 0.0, 0.0 }, |
196
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{ 1, 1, 0, -2, 1, -1.0, 0.0, 0.0, 0.0 }, |
197
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{ 1, 0, -2, 2, 0, -1.0, 0.0, 0.0, 0.0 }, |
198
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{ 2, 0, 0, 2, 0, 1.0, 0.0, 0.0, 0.0 }, |
199
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{ 0, 0, 2, 4, 2, -1.0, 0.0, 0.0, 0.0 }, |
200
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{ 0, 1, 0, 1, 0, 1.0, 0.0, 0.0, 0.0 } |
201
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}; |
202
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203
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/* Number of terms in the series */ |
204
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const int NT = (int) (sizeof x / sizeof x[0]); |
205
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206
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/* ------------------------------------------------------------------ */ |
207
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208
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/* Interval between fundamental epoch J2000.0 and given date (JC). */ |
209
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0
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t = ((date1 - ERFA_DJ00) + date2) / ERFA_DJC; |
210
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211
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/* --------------------- */ |
212
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/* Fundamental arguments */ |
213
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/* --------------------- */ |
214
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215
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/* Mean longitude of Moon minus mean longitude of Moon's perigee. */ |
216
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0
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|
el = eraAnpm( |
217
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0
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|
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|
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(485866.733 + (715922.633 + (31.310 + 0.064 * t) * t) * t) |
218
|
0
|
|
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|
* ERFA_DAS2R + fmod(1325.0 * t, 1.0) * ERFA_D2PI); |
219
|
|
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|
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|
220
|
|
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/* Mean longitude of Sun minus mean longitude of Sun's perigee. */ |
221
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0
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|
elp = eraAnpm( |
222
|
0
|
|
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(1287099.804 + (1292581.224 + (-0.577 - 0.012 * t) * t) * t) |
223
|
0
|
|
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|
* ERFA_DAS2R + fmod(99.0 * t, 1.0) * ERFA_D2PI); |
224
|
|
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|
|
|
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|
225
|
|
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|
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|
/* Mean longitude of Moon minus mean longitude of Moon's node. */ |
226
|
0
|
|
|
|
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|
f = eraAnpm( |
227
|
0
|
|
|
|
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|
(335778.877 + (295263.137 + (-13.257 + 0.011 * t) * t) * t) |
228
|
0
|
|
|
|
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|
* ERFA_DAS2R + fmod(1342.0 * t, 1.0) * ERFA_D2PI); |
229
|
|
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|
|
|
|
|
230
|
|
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|
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|
/* Mean elongation of Moon from Sun. */ |
231
|
0
|
|
|
|
|
|
d = eraAnpm( |
232
|
0
|
|
|
|
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|
(1072261.307 + (1105601.328 + (-6.891 + 0.019 * t) * t) * t) |
233
|
0
|
|
|
|
|
|
* ERFA_DAS2R + fmod(1236.0 * t, 1.0) * ERFA_D2PI); |
234
|
|
|
|
|
|
|
|
235
|
|
|
|
|
|
|
/* Longitude of the mean ascending node of the lunar orbit on the */ |
236
|
|
|
|
|
|
|
/* ecliptic, measured from the mean equinox of date. */ |
237
|
0
|
|
|
|
|
|
om = eraAnpm( |
238
|
0
|
|
|
|
|
|
(450160.280 + (-482890.539 + (7.455 + 0.008 * t) * t) * t) |
239
|
0
|
|
|
|
|
|
* ERFA_DAS2R + fmod(-5.0 * t, 1.0) * ERFA_D2PI); |
240
|
|
|
|
|
|
|
|
241
|
|
|
|
|
|
|
/* --------------- */ |
242
|
|
|
|
|
|
|
/* Nutation series */ |
243
|
|
|
|
|
|
|
/* --------------- */ |
244
|
|
|
|
|
|
|
|
245
|
|
|
|
|
|
|
/* Initialize nutation components. */ |
246
|
|
|
|
|
|
|
dp = 0.0; |
247
|
|
|
|
|
|
|
de = 0.0; |
248
|
|
|
|
|
|
|
|
249
|
|
|
|
|
|
|
/* Sum the nutation terms, ending with the biggest. */ |
250
|
0
|
0
|
|
|
|
|
for (j = NT-1; j >= 0; j--) { |
251
|
|
|
|
|
|
|
|
252
|
|
|
|
|
|
|
/* Form argument for current term. */ |
253
|
0
|
|
|
|
|
|
arg = (double)x[j].nl * el |
254
|
0
|
|
|
|
|
|
+ (double)x[j].nlp * elp |
255
|
0
|
|
|
|
|
|
+ (double)x[j].nf * f |
256
|
0
|
|
|
|
|
|
+ (double)x[j].nd * d |
257
|
0
|
|
|
|
|
|
+ (double)x[j].nom * om; |
258
|
|
|
|
|
|
|
|
259
|
|
|
|
|
|
|
/* Accumulate current nutation term. */ |
260
|
0
|
|
|
|
|
|
s = x[j].sp + x[j].spt * t; |
261
|
0
|
|
|
|
|
|
c = x[j].ce + x[j].cet * t; |
262
|
0
|
0
|
|
|
|
|
if (s != 0.0) dp += s * sin(arg); |
263
|
0
|
0
|
|
|
|
|
if (c != 0.0) de += c * cos(arg); |
264
|
|
|
|
|
|
|
} |
265
|
|
|
|
|
|
|
|
266
|
|
|
|
|
|
|
/* Convert results from 0.1 mas units to radians. */ |
267
|
0
|
|
|
|
|
|
*dpsi = dp * U2R; |
268
|
0
|
|
|
|
|
|
*deps = de * U2R; |
269
|
|
|
|
|
|
|
|
270
|
0
|
|
|
|
|
|
return; |
271
|
|
|
|
|
|
|
|
272
|
|
|
|
|
|
|
} |
273
|
|
|
|
|
|
|
/*---------------------------------------------------------------------- |
274
|
|
|
|
|
|
|
** |
275
|
|
|
|
|
|
|
** |
276
|
|
|
|
|
|
|
** Copyright (C) 2013-2020, NumFOCUS Foundation. |
277
|
|
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|
|
|
|
** All rights reserved. |
278
|
|
|
|
|
|
|
** |
279
|
|
|
|
|
|
|
** This library is derived, with permission, from the International |
280
|
|
|
|
|
|
|
** Astronomical Union's "Standards of Fundamental Astronomy" library, |
281
|
|
|
|
|
|
|
** available from http://www.iausofa.org. |
282
|
|
|
|
|
|
|
** |
283
|
|
|
|
|
|
|
** The ERFA version is intended to retain identical functionality to |
284
|
|
|
|
|
|
|
** the SOFA library, but made distinct through different function and |
285
|
|
|
|
|
|
|
** file names, as set out in the SOFA license conditions. The SOFA |
286
|
|
|
|
|
|
|
** original has a role as a reference standard for the IAU and IERS, |
287
|
|
|
|
|
|
|
** and consequently redistribution is permitted only in its unaltered |
288
|
|
|
|
|
|
|
** state. The ERFA version is not subject to this restriction and |
289
|
|
|
|
|
|
|
** therefore can be included in distributions which do not support the |
290
|
|
|
|
|
|
|
** concept of "read only" software. |
291
|
|
|
|
|
|
|
** |
292
|
|
|
|
|
|
|
** Although the intent is to replicate the SOFA API (other than |
293
|
|
|
|
|
|
|
** replacement of prefix names) and results (with the exception of |
294
|
|
|
|
|
|
|
** bugs; any that are discovered will be fixed), SOFA is not |
295
|
|
|
|
|
|
|
** responsible for any errors found in this version of the library. |
296
|
|
|
|
|
|
|
** |
297
|
|
|
|
|
|
|
** If you wish to acknowledge the SOFA heritage, please acknowledge |
298
|
|
|
|
|
|
|
** that you are using a library derived from SOFA, rather than SOFA |
299
|
|
|
|
|
|
|
** itself. |
300
|
|
|
|
|
|
|
** |
301
|
|
|
|
|
|
|
** |
302
|
|
|
|
|
|
|
** TERMS AND CONDITIONS |
303
|
|
|
|
|
|
|
** |
304
|
|
|
|
|
|
|
** Redistribution and use in source and binary forms, with or without |
305
|
|
|
|
|
|
|
** modification, are permitted provided that the following conditions |
306
|
|
|
|
|
|
|
** are met: |
307
|
|
|
|
|
|
|
** |
308
|
|
|
|
|
|
|
** 1 Redistributions of source code must retain the above copyright |
309
|
|
|
|
|
|
|
** notice, this list of conditions and the following disclaimer. |
310
|
|
|
|
|
|
|
** |
311
|
|
|
|
|
|
|
** 2 Redistributions in binary form must reproduce the above copyright |
312
|
|
|
|
|
|
|
** notice, this list of conditions and the following disclaimer in |
313
|
|
|
|
|
|
|
** the documentation and/or other materials provided with the |
314
|
|
|
|
|
|
|
** distribution. |
315
|
|
|
|
|
|
|
** |
316
|
|
|
|
|
|
|
** 3 Neither the name of the Standards Of Fundamental Astronomy Board, |
317
|
|
|
|
|
|
|
** the International Astronomical Union nor the names of its |
318
|
|
|
|
|
|
|
** contributors may be used to endorse or promote products derived |
319
|
|
|
|
|
|
|
** from this software without specific prior written permission. |
320
|
|
|
|
|
|
|
** |
321
|
|
|
|
|
|
|
** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS |
322
|
|
|
|
|
|
|
** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT |
323
|
|
|
|
|
|
|
** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS |
324
|
|
|
|
|
|
|
** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE |
325
|
|
|
|
|
|
|
** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, |
326
|
|
|
|
|
|
|
** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, |
327
|
|
|
|
|
|
|
** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; |
328
|
|
|
|
|
|
|
** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER |
329
|
|
|
|
|
|
|
** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT |
330
|
|
|
|
|
|
|
** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN |
331
|
|
|
|
|
|
|
** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE |
332
|
|
|
|
|
|
|
** POSSIBILITY OF SUCH DAMAGE. |
333
|
|
|
|
|
|
|
** |
334
|
|
|
|
|
|
|
*/ |