| 1 | /* DeltaT = Ephemeris Time - Universal Time
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| 2 | *
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| 3 | * original code by Stephen Moshier <moshier@world.std.com>,
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| 4 | * adapted to xephem by Michael Sternberg <sternberg@physik.tu-chemnitz.de>
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| 5 | * smoothed transitions and updated by Neal McBurnett <nealmcb@bell-labs.com>
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| 6 | *
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| 7 | **********************************************************************
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| 8 | *
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| 9 | * The tabulated values of deltaT, in hundredths of a second,
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| 10 | * were taken from The Astronomical Almanac, page K8. The program
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| 11 | * adjusts for a value of secular tidal acceleration ndot = -25.8
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| 12 | * arcsec per century squared, the value used in JPL's DE403 ephemeris.
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| 13 | * ELP2000 (and DE200) used the value -23.8946.
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| 14 | *
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| 15 | * The tabulated range is 1620.0 through 1998.0. Bessel's interpolation
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| 16 | * formula is implemented to obtain fourth order interpolated values at
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| 17 | * intermediate times.
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| 18 | *
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| 19 | * For dates earlier than the tabulated range, the program
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| 20 | * calculates approximate formulae of Stephenson and Morrison
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| 21 | * or K. M. Borkowski. These approximations have an estimated
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| 22 | * error of 15 minutes at 1500 B.C. They are not adjusted for small
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| 23 | * improvements in the current estimate of ndot because the formulas
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| 24 | * were derived from studies of ancient eclipses and other historical
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| 25 | * information, whose interpretation depends only partly on ndot.
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| 26 | *
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| 27 | * For future vaues of deltaT, the function smoothly transitions with
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| 28 | * a linear segment back to Stephenson & Morrison's quadratic formula
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| 29 | * in 2130.
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| 30 | *
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| 31 | * Input is mjd (modified julian date from MJD0 on). [stern]
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| 32 | * Note that xephem uses a different epoch for this "mjd" than the
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| 33 | * normal value of JD=240000.5.
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| 34 | * See AA page B4.
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| 35 | *
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| 36 | * Output double deltat(mjd) is ET-UT1 in seconds.
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| 37 | *
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| 38 | *
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| 39 | * References:
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| 40 | *
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| 41 | * Stephenson, F. R., and L. V. Morrison, "Long-term changes
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| 42 | * in the rotation of the Earth: 700 B.C. to A.D. 1980,"
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| 43 | * Philosophical Transactions of the Royal Society of London
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| 44 | * Series A 313, 47-70 (1984)
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| 45 | *
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| 46 | * Borkowski, K. M., "ELP2000-85 and the Dynamical Time
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| 47 | * - Universal Time relation," Astronomy and Astrophysics
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| 48 | * 205, L8-L10 (1988)
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| 49 | * Borkowski's formula is derived from eclipses going back to 2137 BC
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| 50 | * and uses lunar position based on tidal coefficient of -23.9 arcsec/cy^2.
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| 51 | *
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| 52 | * Chapront-Touze, Michelle, and Jean Chapront, _Lunar Tables
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| 53 | * and Programs from 4000 B.C. to A.D. 8000_, Willmann-Bell 1991
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| 54 | * Their table agrees with the one here, but the entries are
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| 55 | * rounded to the nearest whole second.
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| 56 | *
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| 57 | * Stephenson, F. R., and M. A. Houlden, _Atlas of Historical
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| 58 | * Eclipse Maps_, Cambridge U. Press (1986)
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| 59 | *
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| 60 | * from obsolete extrapolation code [stern]:
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| 61 | * Morrison, L. V. and F. R. Stephenson, "Sun and Planetary System"
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| 62 | * vol 96,73 eds. W. Fricke, G. Teleki, Reidel, Dordrecht (1982)
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| 63 | *
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| 64 | **********************************************************************
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| 65 | *
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| 66 | * changes by stern:
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| 67 | * - adopted #include's for xephem
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| 68 | * - made dt[] static
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| 69 | * - made mjd the time argument [was: year Y].
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| 70 | * - updated observed and extrapolated data from tables at
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| 71 | * ftp://maia.usno.navy.mil/ser7/ -- data deviated by up to 0.8 s
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| 72 | * - removed references to "extern double dtgiven"
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| 73 | * - removed DEMO #define and its references
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| 74 | * - replaced treatment after TABEND by linear extrapolation instead
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| 75 | * of second order version
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| 76 | * - installed lastmjd cache (made ans static)
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| 77 | *
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| 78 | * - no changes to table interpolation scheme and past extrapolations */
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| 79 |
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| 80 | #include "P_.h"
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| 81 | #include "astro.h"
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| 82 |
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| 83 | #define TABSTART 1620.0
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| 84 | #define TABEND 2006.0
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| 85 | #define TABSIZ 387
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| 86 |
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| 87 | /* Note, Stephenson and Morrison's table starts at the year 1630.
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| 88 | * The Chapronts' table does not agree with the Almanac prior to 1630.
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| 89 | * The actual accuracy decreases rapidly prior to 1780.
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| 90 | */
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| 91 | static short dt[TABSIZ] = {
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| 92 | /* 1620.0 thru 1659.0 */
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| 93 | 12400, 11900, 11500, 11000, 10600, 10200, 9800, 9500, 9100, 8800,
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| 94 | 8500, 8200, 7900, 7700, 7400, 7200, 7000, 6700, 6500, 6300,
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| 95 | 6200, 6000, 5800, 5700, 5500, 5400, 5300, 5100, 5000, 4900,
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| 96 | 4800, 4700, 4600, 4500, 4400, 4300, 4200, 4100, 4000, 3800,
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| 97 | /* 1660.0 thru 1699.0 */
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| 98 | 3700, 3600, 3500, 3400, 3300, 3200, 3100, 3000, 2800, 2700,
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| 99 | 2600, 2500, 2400, 2300, 2200, 2100, 2000, 1900, 1800, 1700,
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| 100 | 1600, 1500, 1400, 1400, 1300, 1200, 1200, 1100, 1100, 1000,
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| 101 | 1000, 1000, 900, 900, 900, 900, 900, 900, 900, 900,
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| 102 | /* 1700.0 thru 1739.0 */
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| 103 | 900, 900, 900, 900, 900, 900, 900, 900, 1000, 1000,
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| 104 | 1000, 1000, 1000, 1000, 1000, 1000, 1000, 1100, 1100, 1100,
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| 105 | 1100, 1100, 1100, 1100, 1100, 1100, 1100, 1100, 1100, 1100,
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| 106 | 1100, 1100, 1100, 1100, 1200, 1200, 1200, 1200, 1200, 1200,
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| 107 | /* 1740.0 thru 1779.0 */
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| 108 | 1200, 1200, 1200, 1200, 1300, 1300, 1300, 1300, 1300, 1300,
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| 109 | 1300, 1400, 1400, 1400, 1400, 1400, 1400, 1400, 1500, 1500,
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| 110 | 1500, 1500, 1500, 1500, 1500, 1600, 1600, 1600, 1600, 1600,
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| 111 | 1600, 1600, 1600, 1600, 1600, 1700, 1700, 1700, 1700, 1700,
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| 112 | /* 1780.0 thru 1799.0 */
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| 113 | 1700, 1700, 1700, 1700, 1700, 1700, 1700, 1700, 1700, 1700,
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| 114 | 1700, 1700, 1600, 1600, 1600, 1600, 1500, 1500, 1400, 1400,
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| 115 | /* 1800.0 thru 1819.0 */
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| 116 | 1370, 1340, 1310, 1290, 1270, 1260, 1250, 1250, 1250, 1250,
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| 117 | 1250, 1250, 1250, 1250, 1250, 1250, 1250, 1240, 1230, 1220,
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| 118 | /* 1820.0 thru 1859.0 */
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| 119 | 1200, 1170, 1140, 1110, 1060, 1020, 960, 910, 860, 800,
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| 120 | 750, 700, 660, 630, 600, 580, 570, 560, 560, 560,
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| 121 | 570, 580, 590, 610, 620, 630, 650, 660, 680, 690,
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| 122 | 710, 720, 730, 740, 750, 760, 770, 770, 780, 780,
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| 123 | /* 1860.0 thru 1899.0 */
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| 124 | 788, 782, 754, 697, 640, 602, 541, 410, 292, 182,
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| 125 | 161, 10, -102, -128, -269, -324, -364, -454, -471, -511,
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| 126 | -540, -542, -520, -546, -546, -579, -563, -564, -580, -566,
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| 127 | -587, -601, -619, -664, -644, -647, -609, -576, -466, -374,
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| 128 | /* 1900.0 thru 1939.0 */
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| 129 | -272, -154, -2, 124, 264, 386, 537, 614, 775, 913,
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| 130 | 1046, 1153, 1336, 1465, 1601, 1720, 1824, 1906, 2025, 2095,
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| 131 | 2116, 2225, 2241, 2303, 2349, 2362, 2386, 2449, 2434, 2408,
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| 132 | 2402, 2400, 2387, 2395, 2386, 2393, 2373, 2392, 2396, 2402,
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| 133 | /* 1940.0 thru 1979.0 */
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| 134 | 2433, 2483, 2530, 2570, 2624, 2677, 2728, 2778, 2825, 2871,
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| 135 | 2915, 2957, 2997, 3036, 3072, 3107, 3135, 3168, 3218, 3268,
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| 136 | 3315, 3359, 3400, 3447, 3503, 3573, 3654, 3743, 3829, 3920,
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| 137 | 4018, 4117, 4223, 4337, 4449, 4548, 4646, 4752, 4853, 4959,
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| 138 | /* 1980.0 thru 1995.0 */
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| 139 | 5054, 5138, 5217, 5296, 5379, 5434, 5487, 5532, 5582, 5630,
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| 140 | 5686, 5757, 5831, 5912, 5998, 6078,
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| 141 | /* new USNO data (stern) */
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| 142 | 6163, 6230,
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| 143 | /* 1999 USNO data 1998.0 thru 2000.0 (McBurnett) */
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| 144 | 6297, 6347, 6383,
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| 145 | /* 1999 extrapolation (McBurnett), 2001.0 thru 2006.0
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| 146 | Ramp up to 1.6 s/yr to transition smoothly to Stevenson formula
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| 147 | in 2130.0 */
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| 148 | 6440, 6510, 6600, 6750, 6900, 7060
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| 149 |
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| 150 | /* original 1997 USNO extrapolation (stern), 1998.0 thru 2004.0
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| 151 | 6296, 6420,
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| 152 | 6510, 6600, 6700, 6800, 6900 */ /* 7000, 7100, 7200, 7300, 7400, */
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| 153 |
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| 154 | /* Extrapolated values (USNO) (original Moshier) [1996.0 thru 2005.0]
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| 155 | 6183, 6280, 6377, 6475,
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| 156 | 6572, 6667, 6765, 6861, 6957
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| 157 | */
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| 158 | };
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| 159 |
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| 160 | /* calculate DeltaT = ET - UT1 in seconds. Describes the irregularities
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| 161 | * of the Earth rotation rate in the ET time scale.
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| 162 | */
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| 163 | double deltat(mjd)
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| 164 | double mjd;
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| 165 | {
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| 166 | double Y;
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| 167 | double p, B;
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| 168 | int d[6];
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| 169 | int i, iy, k;
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| 170 | double floor();
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| 171 | static double ans;
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| 172 | static double lastmjd = -10000;
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| 173 |
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| 174 | if (mjd == lastmjd) {
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| 175 | return(ans);
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| 176 | }
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| 177 | lastmjd = mjd;
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| 178 |
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| 179 | Y = 2000.0 + (mjd - J2000)/365.25;
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| 180 |
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| 181 | if( Y > TABEND && Y < 2130.0 ) {
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| 182 | /* linear interpolation from table end; stern */
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| 183 | B = Y - TABEND;
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| 184 | ans = dt[TABSIZ-1] + B * (dt[TABSIZ-1] - dt[TABSIZ-2]);
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| 185 | ans *= 0.01;
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| 186 | return(ans);
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| 187 | }
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| 188 |
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| 189 | if( Y < TABSTART || Y >= 2130.0 ) {
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| 190 | if( (Y >= 948.0 - 15.0 && Y < TABSTART) || Y >= 2130.0 ) {
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| 191 | /* Stephenson and Morrison, stated domain is 948 to 1600:
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| 192 | * 25.5(centuries from 1800)^2 - 1.9159(centuries from 1955)^2
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| 193 | * Here we offset by -15 y to minimize the discontinuity,
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| 194 | * thus we use it from 933.0 to 1620.0,
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| 195 | * and from the end of the table to 2130.0.
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| 196 | * f(1620.0) = 60.955200, slope -0.079 s/y
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| 197 | * f(2004.0) = 105.649728, slope 1.02 s/y
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| 198 | * f(2048.0) = 155.176, slope 1.23 s/y
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| 199 | * f(2084.0) = 202.49, slope 1.4 s/y
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| 200 | * f(2130.0) = 272, slope .1616
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| 201 | * f(2150.0) = 305, slope .17
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| 202 | */
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| 203 | B = 0.01*(Y - 2000.0);
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| 204 | ans = (23.58 * B + 100.3)*B + 101.6;
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| 205 | } else {
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| 206 | /* Borkowski */
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| 207 | /* f(2004.0) = 542.7435, slope 2.65 s/y */
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| 208 | B = 0.01*(Y - 2000.0) + 3.75;
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| 209 | ans = 35.0 * B * B + 40.;
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| 210 | }
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| 211 | return(ans);
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| 212 | }
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| 213 |
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| 214 | /* Besselian interpolation from tabulated values.
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| 215 | * See AA page K11.
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| 216 | */
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| 217 |
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| 218 | /* value for 1620.1 is 121.96 or so, not 124.0 */
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| 219 |
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| 220 | /* Index into the table.
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| 221 | */
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| 222 | p = floor(Y);
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| 223 | iy = (int)(p - TABSTART);
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| 224 | /* Zeroth order estimate is value at start of year
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| 225 | */
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| 226 | ans = dt[iy];
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| 227 | k = iy + 1;
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| 228 | if( k >= TABSIZ )
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| 229 | goto done; /* No data, can't go on. */
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| 230 |
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| 231 | /* The fraction of tabulation interval
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| 232 | */
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| 233 | p = Y - p;
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| 234 |
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| 235 | /* First order interpolated value
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| 236 | */
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| 237 | ans += p*(dt[k] - dt[iy]);
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| 238 | if( (iy-1 < 0) || (iy+2 >= TABSIZ) )
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| 239 | goto done; /* can't do second differences */
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| 240 |
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| 241 | /* Make table of first differences
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| 242 | */
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| 243 | k = iy - 2;
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| 244 | for( i=0; i<5; i++ ) {
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| 245 | if( (k < 0) || (k+1 >= TABSIZ) )
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| 246 | d[i] = 0;
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| 247 | else d[i] = dt[k+1] - dt[k];
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| 248 | k += 1;
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| 249 | }
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| 250 |
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| 251 | /* Compute second differences
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| 252 | */
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| 253 | for( i=0; i<4; i++ )
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| 254 | d[i] = d[i+1] - d[i];
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| 255 | B = 0.25*p*(p-1.0);
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| 256 | ans += B*(d[1] + d[2]);
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| 257 | if( iy+2 >= TABSIZ )
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| 258 | goto done;
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| 259 |
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| 260 | /* Compute third differences
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| 261 | */
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| 262 | for( i=0; i<3; i++ )
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| 263 | d[i] = d[i+1] - d[i];
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| 264 | B = 2.0*B/3.0;
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| 265 | ans += (p-0.5)*B*d[1];
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| 266 | if( (iy-2 < 0) || (iy+3 > TABSIZ) )
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| 267 | goto done;
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| 268 |
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| 269 | /* Compute fourth differences
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| 270 | */
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| 271 | for( i=0; i<2; i++ )
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| 272 | d[i] = d[i+1] - d[i];
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| 273 | B = 0.125*B*(p+1.0)*(p-2.0);
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| 274 | ans += B*(d[0] + d[1]);
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| 275 |
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| 276 | done:
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| 277 | /* Astronomical Almanac table is corrected by adding the expression
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| 278 | * -0.000091 (ndot + 26)(year-1955)^2 seconds
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| 279 | * to entries prior to 1955 (AA page K8), where ndot is the secular
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| 280 | * tidal term in the mean motion of the Moon.
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| 281 | *
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| 282 | * Entries after 1955 are referred to atomic time standards and
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| 283 | * are not affected by errors in Lunar or planetary theory.
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| 284 | */
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| 285 | ans *= 0.01;
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| 286 | if( Y < 1955.0 ) {
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| 287 | B = (Y - 1955.0);
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| 288 | ans += -0.000091 * (-25.8 + 26.0) * B * B;
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| 289 | }
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| 290 | return( ans );
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| 291 | }
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| 292 |
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| 293 |
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| 294 | #ifdef TEST_DT
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| 295 | main()
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| 296 | {
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| 297 | double ans, y;
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| 298 |
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| 299 | while (scanf("%lf", &y) == 1) {
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| 300 | ans = deltat((y - 2000.0)*365.25 + J2000);
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| 301 | printf("%.4lf %.4lf\n", y, ans);
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| 302 | }
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| 303 | }
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| 304 | #endif
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| 305 |
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| 306 | /* For RCS Only -- Do Not Edit */
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| 307 | static char *rcsid[2] = {(char *)rcsid, "@(#) $RCSfile: deltat.c,v $ $Date: 2001-04-10 14:40:46 $ $Revision: 1.1.1.1 $ $Name: not supported by cvs2svn $"};
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