| 1 | #include "erfa.h"
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| 2 | #include <string.h>
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| 3 |
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| 4 | int eraD2dtf(const char *scale, int ndp, double d1, double d2,
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| 5 | int *iy, int *im, int *id, int ihmsf[4])
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| 6 | /*
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| 7 | ** - - - - - - - - -
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| 8 | ** e r a D 2 d t f
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| 9 | ** - - - - - - - - -
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| 10 | **
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| 11 | ** Format for output a 2-part Julian Date (or in the case of UTC a
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| 12 | ** quasi-JD form that includes special provision for leap seconds).
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| 13 | **
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| 14 | ** Given:
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| 15 | ** scale char[] time scale ID (Note 1)
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| 16 | ** ndp int resolution (Note 2)
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| 17 | ** d1,d2 double time as a 2-part Julian Date (Notes 3,4)
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| 18 | **
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| 19 | ** Returned:
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| 20 | ** iy,im,id int year, month, day in Gregorian calendar (Note 5)
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| 21 | ** ihmsf int[4] hours, minutes, seconds, fraction (Note 1)
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| 22 | **
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| 23 | ** Returned (function value):
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| 24 | ** int status: +1 = dubious year (Note 5)
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| 25 | ** 0 = OK
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| 26 | ** -1 = unacceptable date (Note 6)
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| 27 | **
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| 28 | ** Notes:
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| 29 | **
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| 30 | ** 1) scale identifies the time scale. Only the value "UTC" (in upper
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| 31 | ** case) is significant, and enables handling of leap seconds (see
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| 32 | ** Note 4).
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| 33 | **
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| 34 | ** 2) ndp is the number of decimal places in the seconds field, and can
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| 35 | ** have negative as well as positive values, such as:
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| 36 | **
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| 37 | ** ndp resolution
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| 38 | ** -4 1 00 00
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| 39 | ** -3 0 10 00
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| 40 | ** -2 0 01 00
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| 41 | ** -1 0 00 10
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| 42 | ** 0 0 00 01
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| 43 | ** 1 0 00 00.1
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| 44 | ** 2 0 00 00.01
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| 45 | ** 3 0 00 00.001
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| 46 | **
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| 47 | ** The limits are platform dependent, but a safe range is -5 to +9.
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| 48 | **
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| 49 | ** 3) d1+d2 is Julian Date, apportioned in any convenient way between
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| 50 | ** the two arguments, for example where d1 is the Julian Day Number
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| 51 | ** and d2 is the fraction of a day. In the case of UTC, where the
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| 52 | ** use of JD is problematical, special conventions apply: see the
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| 53 | ** next note.
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| 54 | **
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| 55 | ** 4) JD cannot unambiguously represent UTC during a leap second unless
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| 56 | ** special measures are taken. The ERFA internal convention is that
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| 57 | ** the quasi-JD day represents UTC days whether the length is 86399,
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| 58 | ** 86400 or 86401 SI seconds. In the 1960-1972 era there were
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| 59 | ** smaller jumps (in either direction) each time the linear UTC(TAI)
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| 60 | ** expression was changed, and these "mini-leaps" are also included
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| 61 | ** in the ERFA convention.
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| 62 | **
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| 63 | ** 5) The warning status "dubious year" flags UTCs that predate the
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| 64 | ** introduction of the time scale or that are too far in the future
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| 65 | ** to be trusted. See eraDat for further details.
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| 66 | **
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| 67 | ** 6) For calendar conventions and limitations, see eraCal2jd.
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| 68 | **
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| 69 | ** Called:
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| 70 | ** eraJd2cal JD to Gregorian calendar
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| 71 | ** eraD2tf decompose days to hms
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| 72 | ** eraDat delta(AT) = TAI-UTC
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| 73 | **
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| 74 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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| 75 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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| 76 | */
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| 77 | {
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| 78 | int leap;
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| 79 | char s;
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| 80 | int iy1, im1, id1, js, iy2, im2, id2, ihmsf1[4], i;
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| 81 | double a1, b1, fd, dat0, dat12, w, dat24, dleap;
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| 82 |
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| 83 |
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| 84 | /* The two-part JD. */
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| 85 | a1 = d1;
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| 86 | b1 = d2;
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| 87 |
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| 88 | /* Provisional calendar date. */
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| 89 | js = eraJd2cal(a1, b1, &iy1, &im1, &id1, &fd);
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| 90 | if ( js ) return -1;
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| 91 |
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| 92 | /* Is this a leap second day? */
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| 93 | leap = 0;
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| 94 | if ( ! strcmp(scale,"UTC") ) {
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| 95 |
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| 96 | /* TAI-UTC at 0h today. */
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| 97 | js = eraDat(iy1, im1, id1, 0.0, &dat0);
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| 98 | if ( js < 0 ) return -1;
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| 99 |
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| 100 | /* TAI-UTC at 12h today (to detect drift). */
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| 101 | js = eraDat(iy1, im1, id1, 0.5, &dat12);
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| 102 | if ( js < 0 ) return -1;
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| 103 |
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| 104 | /* TAI-UTC at 0h tomorrow (to detect jumps). */
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| 105 | js = eraJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
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| 106 | if ( js ) return -1;
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| 107 | js = eraDat(iy2, im2, id2, 0.0, &dat24);
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| 108 | if ( js < 0 ) return -1;
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| 109 |
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| 110 | /* Any sudden change in TAI-UTC (seconds). */
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| 111 | dleap = dat24 - (2.0*dat12 - dat0);
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| 112 |
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| 113 | /* If leap second day, scale the fraction of a day into SI. */
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| 114 | leap = (dleap != 0.0);
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| 115 | if (leap) fd += fd * dleap/ERFA_DAYSEC;
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| 116 | }
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| 117 |
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| 118 | /* Provisional time of day. */
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| 119 | eraD2tf ( ndp, fd, &s, ihmsf1 );
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| 120 |
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| 121 | /* Has the (rounded) time gone past 24h? */
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| 122 | if ( ihmsf1[0] > 23 ) {
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| 123 |
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| 124 | /* Yes. We probably need tomorrow's calendar date. */
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| 125 | js = eraJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
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| 126 | if ( js ) return -1;
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| 127 |
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| 128 | /* Is today a leap second day? */
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| 129 | if ( ! leap ) {
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| 130 |
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| 131 | /* No. Use 0h tomorrow. */
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| 132 | iy1 = iy2;
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| 133 | im1 = im2;
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| 134 | id1 = id2;
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| 135 | ihmsf1[0] = 0;
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| 136 | ihmsf1[1] = 0;
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| 137 | ihmsf1[2] = 0;
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| 138 |
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| 139 | } else {
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| 140 |
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| 141 | /* Yes. Are we past the leap second itself? */
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| 142 | if ( ihmsf1[2] > 0 ) {
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| 143 |
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| 144 | /* Yes. Use tomorrow but allow for the leap second. */
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| 145 | iy1 = iy2;
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| 146 | im1 = im2;
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| 147 | id1 = id2;
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| 148 | ihmsf1[0] = 0;
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| 149 | ihmsf1[1] = 0;
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| 150 | ihmsf1[2] = 0;
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| 151 |
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| 152 | } else {
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| 153 |
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| 154 | /* No. Use 23 59 60... today. */
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| 155 | ihmsf1[0] = 23;
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| 156 | ihmsf1[1] = 59;
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| 157 | ihmsf1[2] = 60;
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| 158 | }
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| 159 |
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| 160 | /* If rounding to 10s or coarser always go up to new day. */
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| 161 | if ( ndp < 0 && ihmsf1[2] == 60 ) {
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| 162 | iy1 = iy2;
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| 163 | im1 = im2;
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| 164 | id1 = id2;
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| 165 | ihmsf1[0] = 0;
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| 166 | ihmsf1[1] = 0;
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| 167 | ihmsf1[2] = 0;
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| 168 | }
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| 169 | }
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| 170 | }
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| 171 |
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| 172 | /* Results. */
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| 173 | *iy = iy1;
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| 174 | *im = im1;
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| 175 | *id = id1;
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| 176 | for ( i = 0; i < 4; i++ ) {
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| 177 | ihmsf[i] = ihmsf1[i];
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| 178 | }
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| 179 |
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| 180 | /* Status. */
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| 181 | return js;
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| 182 |
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| 183 | }
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| 184 | /*----------------------------------------------------------------------
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| 185 | **
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| 186 | **
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| 187 | ** Copyright (C) 2013-2017, NumFOCUS Foundation.
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| 188 | ** All rights reserved.
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| 189 | **
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| 190 | ** This library is derived, with permission, from the International
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| 191 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 192 | ** available from http://www.iausofa.org.
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| 193 | **
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| 194 | ** The ERFA version is intended to retain identical functionality to
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| 195 | ** the SOFA library, but made distinct through different function and
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| 196 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 197 | ** original has a role as a reference standard for the IAU and IERS,
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| 198 | ** and consequently redistribution is permitted only in its unaltered
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| 199 | ** state. The ERFA version is not subject to this restriction and
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| 200 | ** therefore can be included in distributions which do not support the
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| 201 | ** concept of "read only" software.
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| 202 | **
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| 203 | ** Although the intent is to replicate the SOFA API (other than
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| 204 | ** replacement of prefix names) and results (with the exception of
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| 205 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 206 | ** responsible for any errors found in this version of the library.
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| 207 | **
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| 208 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 209 | ** that you are using a library derived from SOFA, rather than SOFA
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| 210 | ** itself.
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| 211 | **
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| 212 | **
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| 213 | ** TERMS AND CONDITIONS
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| 214 | **
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| 215 | ** Redistribution and use in source and binary forms, with or without
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| 216 | ** modification, are permitted provided that the following conditions
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| 217 | ** are met:
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| 218 | **
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| 219 | ** 1 Redistributions of source code must retain the above copyright
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| 220 | ** notice, this list of conditions and the following disclaimer.
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| 221 | **
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| 222 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 223 | ** notice, this list of conditions and the following disclaimer in
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| 224 | ** the documentation and/or other materials provided with the
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| 225 | ** distribution.
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| 226 | **
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| 227 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 228 | ** the International Astronomical Union nor the names of its
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| 229 | ** contributors may be used to endorse or promote products derived
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| 230 | ** from this software without specific prior written permission.
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| 231 | **
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| 232 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 233 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 234 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 235 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 236 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 237 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 238 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 239 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 240 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 241 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 242 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 243 | ** POSSIBILITY OF SUCH DAMAGE.
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| 244 | **
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| 245 | */
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