1 | #include "erfa.h"
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2 |
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3 | int eraJd2cal(double dj1, double dj2,
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4 | int *iy, int *im, int *id, double *fd)
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5 | /*
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6 | ** - - - - - - - - - -
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7 | ** e r a J d 2 c a l
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8 | ** - - - - - - - - - -
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9 | **
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10 | ** Julian Date to Gregorian year, month, day, and fraction of a day.
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11 | **
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12 | ** Given:
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13 | ** dj1,dj2 double Julian Date (Notes 1, 2)
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14 | **
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15 | ** Returned (arguments):
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16 | ** iy int year
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17 | ** im int month
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18 | ** id int day
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19 | ** fd double fraction of day
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20 | **
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21 | ** Returned (function value):
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22 | ** int status:
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23 | ** 0 = OK
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24 | ** -1 = unacceptable date (Note 3)
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25 | **
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26 | ** Notes:
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27 | **
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28 | ** 1) The earliest valid date is -68569.5 (-4900 March 1). The
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29 | ** largest value accepted is 1e9.
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30 | **
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31 | ** 2) The Julian Date is apportioned in any convenient way between
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32 | ** the arguments dj1 and dj2. For example, JD=2450123.7 could
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33 | ** be expressed in any of these ways, among others:
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34 | **
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35 | ** dj1 dj2
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36 | **
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37 | ** 2450123.7 0.0 (JD method)
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38 | ** 2451545.0 -1421.3 (J2000 method)
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39 | ** 2400000.5 50123.2 (MJD method)
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40 | ** 2450123.5 0.2 (date & time method)
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41 | **
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42 | ** 3) In early eras the conversion is from the "proleptic Gregorian
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43 | ** calendar"; no account is taken of the date(s) of adoption of
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44 | ** the Gregorian calendar, nor is the AD/BC numbering convention
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45 | ** observed.
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46 | **
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47 | ** Reference:
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48 | **
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49 | ** Explanatory Supplement to the Astronomical Almanac,
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50 | ** P. Kenneth Seidelmann (ed), University Science Books (1992),
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51 | ** Section 12.92 (p604).
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52 | **
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53 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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54 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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55 | */
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56 | {
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57 | /* Minimum and maximum allowed JD */
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58 | const double DJMIN = -68569.5;
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59 | const double DJMAX = 1e9;
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60 |
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61 | long jd, l, n, i, k;
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62 | double dj, d1, d2, f1, f2, f, d;
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63 |
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64 |
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65 | /* Verify date is acceptable. */
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66 | dj = dj1 + dj2;
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67 | if (dj < DJMIN || dj > DJMAX) return -1;
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68 |
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69 | /* Copy the date, big then small, and re-align to midnight. */
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70 | if (dj1 >= dj2) {
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71 | d1 = dj1;
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72 | d2 = dj2;
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73 | } else {
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74 | d1 = dj2;
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75 | d2 = dj1;
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76 | }
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77 | d2 -= 0.5;
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78 |
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79 | /* Separate day and fraction. */
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80 | f1 = fmod(d1, 1.0);
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81 | f2 = fmod(d2, 1.0);
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82 | f = fmod(f1 + f2, 1.0);
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83 | if (f < 0.0) f += 1.0;
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84 | d = floor(d1 - f1) + floor(d2 - f2) + floor(f1 + f2 - f);
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85 | jd = (long) floor(d) + 1L;
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86 |
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87 | /* Express day in Gregorian calendar. */
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88 | l = jd + 68569L;
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89 | n = (4L * l) / 146097L;
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90 | l -= (146097L * n + 3L) / 4L;
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91 | i = (4000L * (l + 1L)) / 1461001L;
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92 | l -= (1461L * i) / 4L - 31L;
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93 | k = (80L * l) / 2447L;
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94 | *id = (int) (l - (2447L * k) / 80L);
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95 | l = k / 11L;
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96 | *im = (int) (k + 2L - 12L * l);
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97 | *iy = (int) (100L * (n - 49L) + i + l);
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98 | *fd = f;
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99 |
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100 | return 0;
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101 |
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102 | }
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103 | /*----------------------------------------------------------------------
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104 | **
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105 | **
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106 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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107 | ** All rights reserved.
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108 | **
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109 | ** This library is derived, with permission, from the International
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110 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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111 | ** available from http://www.iausofa.org.
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112 | **
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113 | ** The ERFA version is intended to retain identical functionality to
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114 | ** the SOFA library, but made distinct through different function and
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115 | ** file names, as set out in the SOFA license conditions. The SOFA
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116 | ** original has a role as a reference standard for the IAU and IERS,
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117 | ** and consequently redistribution is permitted only in its unaltered
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118 | ** state. The ERFA version is not subject to this restriction and
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119 | ** therefore can be included in distributions which do not support the
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120 | ** concept of "read only" software.
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121 | **
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122 | ** Although the intent is to replicate the SOFA API (other than
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123 | ** replacement of prefix names) and results (with the exception of
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124 | ** bugs; any that are discovered will be fixed), SOFA is not
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125 | ** responsible for any errors found in this version of the library.
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126 | **
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127 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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128 | ** that you are using a library derived from SOFA, rather than SOFA
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129 | ** itself.
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130 | **
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131 | **
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132 | ** TERMS AND CONDITIONS
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133 | **
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134 | ** Redistribution and use in source and binary forms, with or without
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135 | ** modification, are permitted provided that the following conditions
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136 | ** are met:
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137 | **
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138 | ** 1 Redistributions of source code must retain the above copyright
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139 | ** notice, this list of conditions and the following disclaimer.
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140 | **
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141 | ** 2 Redistributions in binary form must reproduce the above copyright
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142 | ** notice, this list of conditions and the following disclaimer in
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143 | ** the documentation and/or other materials provided with the
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144 | ** distribution.
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145 | **
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146 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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147 | ** the International Astronomical Union nor the names of its
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148 | ** contributors may be used to endorse or promote products derived
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149 | ** from this software without specific prior written permission.
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150 | **
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151 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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152 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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153 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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154 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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155 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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156 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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157 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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158 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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159 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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160 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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161 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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162 | ** POSSIBILITY OF SUCH DAMAGE.
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163 | **
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164 | */
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