1 | #include "erfa.h"
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2 | #include <string.h>
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3 |
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4 | int eraDtf2d(const char *scale, int iy, int im, int id,
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5 | int ihr, int imn, double sec, double *d1, double *d2)
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6 | /*
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7 | ** - - - - - - - - -
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8 | ** e r a D t f 2 d
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9 | ** - - - - - - - - -
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10 | **
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11 | ** Encode date and time fields into 2-part Julian Date (or in the case
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12 | ** of UTC a quasi-JD form that includes special provision for leap
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13 | ** seconds).
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14 | **
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15 | ** Given:
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16 | ** scale char[] time scale ID (Note 1)
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17 | ** iy,im,id int year, month, day in Gregorian calendar (Note 2)
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18 | ** ihr,imn int hour, minute
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19 | ** sec double seconds
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20 | **
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21 | ** Returned:
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22 | ** d1,d2 double 2-part Julian Date (Notes 3,4)
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23 | **
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24 | ** Returned (function value):
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25 | ** int status: +3 = both of next two
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26 | ** +2 = time is after end of day (Note 5)
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27 | ** +1 = dubious year (Note 6)
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28 | ** 0 = OK
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29 | ** -1 = bad year
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30 | ** -2 = bad month
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31 | ** -3 = bad day
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32 | ** -4 = bad hour
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33 | ** -5 = bad minute
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34 | ** -6 = bad second (<0)
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35 | **
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36 | ** Notes:
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37 | **
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38 | ** 1) scale identifies the time scale. Only the value "UTC" (in upper
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39 | ** case) is significant, and enables handling of leap seconds (see
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40 | ** Note 4).
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41 | **
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42 | ** 2) For calendar conventions and limitations, see eraCal2jd.
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43 | **
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44 | ** 3) The sum of the results, d1+d2, is Julian Date, where normally d1
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45 | ** is the Julian Day Number and d2 is the fraction of a day. In the
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46 | ** case of UTC, where the use of JD is problematical, special
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47 | ** conventions apply: see the next note.
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48 | **
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49 | ** 4) JD cannot unambiguously represent UTC during a leap second unless
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50 | ** special measures are taken. The ERFA internal convention is that
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51 | ** the quasi-JD day represents UTC days whether the length is 86399,
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52 | ** 86400 or 86401 SI seconds. In the 1960-1972 era there were
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53 | ** smaller jumps (in either direction) each time the linear UTC(TAI)
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54 | ** expression was changed, and these "mini-leaps" are also included
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55 | ** in the ERFA convention.
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56 | **
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57 | ** 5) The warning status "time is after end of day" usually means that
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58 | ** the sec argument is greater than 60.0. However, in a day ending
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59 | ** in a leap second the limit changes to 61.0 (or 59.0 in the case
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60 | ** of a negative leap second).
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61 | **
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62 | ** 6) The warning status "dubious year" flags UTCs that predate the
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63 | ** introduction of the time scale or that are too far in the future
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64 | ** to be trusted. See eraDat for further details.
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65 | **
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66 | ** 7) Only in the case of continuous and regular time scales (TAI, TT,
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67 | ** TCG, TCB and TDB) is the result d1+d2 a Julian Date, strictly
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68 | ** speaking. In the other cases (UT1 and UTC) the result must be
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69 | ** used with circumspection; in particular the difference between
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70 | ** two such results cannot be interpreted as a precise time
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71 | ** interval.
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72 | **
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73 | ** Called:
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74 | ** eraCal2jd Gregorian calendar to JD
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75 | ** eraDat delta(AT) = TAI-UTC
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76 | ** eraJd2cal JD to Gregorian calendar
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77 | **
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78 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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79 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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80 | */
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81 | {
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82 | int js, iy2, im2, id2;
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83 | double dj, w, day, seclim, dat0, dat12, dat24, dleap, time;
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84 |
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85 |
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86 | /* Today's Julian Day Number. */
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87 | js = eraCal2jd(iy, im, id, &dj, &w);
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88 | if ( js ) return js;
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89 | dj += w;
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90 |
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91 | /* Day length and final minute length in seconds (provisional). */
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92 | day = ERFA_DAYSEC;
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93 | seclim = 60.0;
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94 |
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95 | /* Deal with the UTC leap second case. */
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96 | if ( ! strcmp(scale,"UTC") ) {
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97 |
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98 | /* TAI-UTC at 0h today. */
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99 | js = eraDat(iy, im, id, 0.0, &dat0);
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100 | if ( js < 0 ) return js;
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101 |
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102 | /* TAI-UTC at 12h today (to detect drift). */
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103 | js = eraDat(iy, im, id, 0.5, &dat12);
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104 | if ( js < 0 ) return js;
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105 |
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106 | /* TAI-UTC at 0h tomorrow (to detect jumps). */
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107 | js = eraJd2cal ( dj, 1.5, &iy2, &im2, &id2, &w);
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108 | if ( js ) return js;
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109 | js = eraDat(iy2, im2, id2, 0.0, &dat24);
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110 | if ( js < 0 ) return js;
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111 |
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112 | /* Any sudden change in TAI-UTC between today and tomorrow. */
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113 | dleap = dat24 - (2.0*dat12 - dat0);
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114 |
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115 | /* If leap second day, correct the day and final minute lengths. */
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116 | day += dleap;
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117 | if ( ihr == 23 && imn == 59 ) seclim += dleap;
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118 |
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119 | /* End of UTC-specific actions. */
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120 | }
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121 |
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122 | /* Validate the time. */
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123 | if ( ihr >= 0 && ihr <= 23 ) {
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124 | if ( imn >= 0 && imn <= 59 ) {
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125 | if ( sec >= 0 ) {
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126 | if ( sec >= seclim ) {
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127 | js += 2;
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128 | }
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129 | } else {
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130 | js = -6;
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131 | }
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132 | } else {
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133 | js = -5;
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134 | }
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135 | } else {
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136 | js = -4;
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137 | }
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138 | if ( js < 0 ) return js;
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139 |
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140 | /* The time in days. */
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141 | time = ( 60.0 * ( (double) ( 60 * ihr + imn ) ) + sec ) / day;
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142 |
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143 | /* Return the date and time. */
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144 | *d1 = dj;
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145 | *d2 = time;
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146 |
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147 | /* Status. */
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148 | return js;
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149 |
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150 | }
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151 | /*----------------------------------------------------------------------
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152 | **
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153 | **
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154 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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155 | ** All rights reserved.
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156 | **
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157 | ** This library is derived, with permission, from the International
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158 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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159 | ** available from http://www.iausofa.org.
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160 | **
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161 | ** The ERFA version is intended to retain identical functionality to
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162 | ** the SOFA library, but made distinct through different function and
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163 | ** file names, as set out in the SOFA license conditions. The SOFA
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164 | ** original has a role as a reference standard for the IAU and IERS,
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165 | ** and consequently redistribution is permitted only in its unaltered
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166 | ** state. The ERFA version is not subject to this restriction and
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167 | ** therefore can be included in distributions which do not support the
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168 | ** concept of "read only" software.
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169 | **
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170 | ** Although the intent is to replicate the SOFA API (other than
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171 | ** replacement of prefix names) and results (with the exception of
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172 | ** bugs; any that are discovered will be fixed), SOFA is not
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173 | ** responsible for any errors found in this version of the library.
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174 | **
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175 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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176 | ** that you are using a library derived from SOFA, rather than SOFA
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177 | ** itself.
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178 | **
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179 | **
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180 | ** TERMS AND CONDITIONS
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181 | **
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182 | ** Redistribution and use in source and binary forms, with or without
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183 | ** modification, are permitted provided that the following conditions
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184 | ** are met:
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185 | **
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186 | ** 1 Redistributions of source code must retain the above copyright
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187 | ** notice, this list of conditions and the following disclaimer.
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188 | **
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189 | ** 2 Redistributions in binary form must reproduce the above copyright
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190 | ** notice, this list of conditions and the following disclaimer in
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191 | ** the documentation and/or other materials provided with the
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192 | ** distribution.
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193 | **
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194 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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195 | ** the International Astronomical Union nor the names of its
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196 | ** contributors may be used to endorse or promote products derived
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197 | ** from this software without specific prior written permission.
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198 | **
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199 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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200 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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201 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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202 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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203 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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204 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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205 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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206 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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207 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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208 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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209 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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210 | ** POSSIBILITY OF SUCH DAMAGE.
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211 | **
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212 | */
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