FACT++
1.0
Main Page
Related Pages
Namespaces
Classes
Files
Examples
File List
File Members
gmst00.c
Go to the documentation of this file.
1
#include "
erfa.h
"
2
3
double
eraGmst00
(
double
uta,
double
utb,
double
tta,
double
ttb)
4
/*
5
** - - - - - - - - - -
6
** e r a G m s t 0 0
7
** - - - - - - - - - -
8
**
9
** Greenwich mean sidereal time (model consistent with IAU 2000
10
** resolutions).
11
**
12
** Given:
13
** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
14
** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
15
**
16
** Returned (function value):
17
** double Greenwich mean sidereal time (radians)
18
**
19
** Notes:
20
**
21
** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
22
** Julian Dates, apportioned in any convenient way between the
23
** argument pairs. For example, JD=2450123.7 could be expressed in
24
** any of these ways, among others:
25
**
26
** Part A Part B
27
**
28
** 2450123.7 0.0 (JD method)
29
** 2451545.0 -1421.3 (J2000 method)
30
** 2400000.5 50123.2 (MJD method)
31
** 2450123.5 0.2 (date & time method)
32
**
33
** The JD method is the most natural and convenient to use in
34
** cases where the loss of several decimal digits of resolution
35
** is acceptable (in the case of UT; the TT is not at all critical
36
** in this respect). The J2000 and MJD methods are good compromises
37
** between resolution and convenience. For UT, the date & time
38
** method is best matched to the algorithm that is used by the Earth
39
** Rotation Angle function, called internally: maximum precision is
40
** delivered when the uta argument is for 0hrs UT1 on the day in
41
** question and the utb argument lies in the range 0 to 1, or vice
42
** versa.
43
**
44
** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
45
** and TT to predict the effects of precession. If UT1 is used for
46
** both purposes, errors of order 100 microarcseconds result.
47
**
48
** 3) This GMST is compatible with the IAU 2000 resolutions and must be
49
** used only in conjunction with other IAU 2000 compatible
50
** components such as precession-nutation and equation of the
51
** equinoxes.
52
**
53
** 4) The result is returned in the range 0 to 2pi.
54
**
55
** 5) The algorithm is from Capitaine et al. (2003) and IERS
56
** Conventions 2003.
57
**
58
** Called:
59
** eraEra00 Earth rotation angle, IAU 2000
60
** eraAnp normalize angle into range 0 to 2pi
61
**
62
** References:
63
**
64
** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
65
** implement the IAU 2000 definition of UT1", Astronomy &
66
** Astrophysics, 406, 1135-1149 (2003)
67
**
68
** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
69
** IERS Technical Note No. 32, BKG (2004)
70
**
71
** Copyright (C) 2013-2015, NumFOCUS Foundation.
72
** Derived, with permission, from the SOFA library. See notes at end of file.
73
*/
74
{
75
double
t
, gmst;
76
77
/* TT Julian centuries since J2000.0. */
78
t = ((tta -
ERFA_DJ00
) + ttb) /
ERFA_DJC
;
79
80
/* Greenwich Mean Sidereal Time, IAU 2000. */
81
gmst =
eraAnp
(
eraEra00
(uta, utb) +
82
( 0.014506 +
83
( 4612.15739966 +
84
( 1.39667721 +
85
( -0.00009344 +
86
( 0.00001882 )
87
* t) * t) * t) * t) *
ERFA_DAS2R
);
88
89
return
gmst;
90
91
}
92
/*----------------------------------------------------------------------
93
**
94
**
95
** Copyright (C) 2013-2015, NumFOCUS Foundation.
96
** All rights reserved.
97
**
98
** This library is derived, with permission, from the International
99
** Astronomical Union's "Standards of Fundamental Astronomy" library,
100
** available from http://www.iausofa.org.
101
**
102
** The ERFA version is intended to retain identical functionality to
103
** the SOFA library, but made distinct through different function and
104
** file names, as set out in the SOFA license conditions. The SOFA
105
** original has a role as a reference standard for the IAU and IERS,
106
** and consequently redistribution is permitted only in its unaltered
107
** state. The ERFA version is not subject to this restriction and
108
** therefore can be included in distributions which do not support the
109
** concept of "read only" software.
110
**
111
** Although the intent is to replicate the SOFA API (other than
112
** replacement of prefix names) and results (with the exception of
113
** bugs; any that are discovered will be fixed), SOFA is not
114
** responsible for any errors found in this version of the library.
115
**
116
** If you wish to acknowledge the SOFA heritage, please acknowledge
117
** that you are using a library derived from SOFA, rather than SOFA
118
** itself.
119
**
120
**
121
** TERMS AND CONDITIONS
122
**
123
** Redistribution and use in source and binary forms, with or without
124
** modification, are permitted provided that the following conditions
125
** are met:
126
**
127
** 1 Redistributions of source code must retain the above copyright
128
** notice, this list of conditions and the following disclaimer.
129
**
130
** 2 Redistributions in binary form must reproduce the above copyright
131
** notice, this list of conditions and the following disclaimer in
132
** the documentation and/or other materials provided with the
133
** distribution.
134
**
135
** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
136
** the International Astronomical Union nor the names of its
137
** contributors may be used to endorse or promote products derived
138
** from this software without specific prior written permission.
139
**
140
** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
141
** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
142
** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
143
** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
144
** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
145
** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
146
** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
147
** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
148
** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
149
** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
150
** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
151
** POSSIBILITY OF SUCH DAMAGE.
152
**
153
*/
ERFA_DJ00
#define ERFA_DJ00
Definition:
erfam.h:87
ERFA_DAS2R
#define ERFA_DAS2R
Definition:
erfam.h:60
eraEra00
double eraEra00(double dj1, double dj2)
Definition:
era00.c:3
ERFA_DJC
#define ERFA_DJC
Definition:
erfam.h:81
erfa.h
t
TT t
Definition:
test_client.c:26
eraAnp
double eraAnp(double a)
Definition:
anp.c:3
eraGmst00
double eraGmst00(double uta, double utb, double tta, double ttb)
Definition:
gmst00.c:3
erfa
src
gmst00.c
Generated on Sun Sep 18 2016 20:50:18 for FACT++ by
1.8.11