1 | #include "slalib.h"
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2 | #include "slamac.h"
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3 | double slaDt ( double epoch )
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4 | /*
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5 | ** - - - - - -
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6 | ** s l a D t
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7 | ** - - - - - -
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8 | **
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9 | ** Estimate the offset between dynamical time and Universal Time
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10 | ** for a given historical epoch.
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11 | **
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12 | ** (double precision)
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13 | **
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14 | ** Given:
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15 | ** epoch double (Julian) epoch (e.g. 1850.0)
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16 | **
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17 | ** The result is a rough estimate of ET-UT (after 1984, TT-UT1) at
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18 | ** the given epoch, in seconds.
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19 | **
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20 | ** Notes:
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21 | **
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22 | ** 1 Depending on the epoch, one of three parabolic approximations
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23 | ** is used:
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24 | **
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25 | ** before 979 Stephenson & Morrison's 390 BC to AD 948 model
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26 | ** 979 to 1708 Stephenson & Morrison's 948 to 1600 model
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27 | ** after 1708 McCarthy & Babcock's post-1650 model
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28 | **
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29 | ** The breakpoints are chosen to ensure continuity: they occur
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30 | ** at places where the adjacent models give the same answer as
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31 | ** each other.
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32 | **
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33 | ** 2 The accuracy is modest, with errors of up to 20 sec during
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34 | ** the interval since 1650, rising to perhaps 30 min by 1000 BC.
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35 | ** Comparatively accurate values from AD 1600 are tabulated in
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36 | ** the Astronomical Almanac (see section K8 of the 1995 AA).
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37 | **
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38 | ** 3 The use of double-precision for both argument and result is
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39 | ** purely for compatibility with other SLALIB time routines.
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40 | **
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41 | ** 4 The models used are based on a lunar tidal acceleration value
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42 | ** of -26.00 arcsec per century.
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43 | **
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44 | ** Reference: Explanatory Supplement to the Astronomical Almanac,
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45 | ** ed P.K.Seidelmann, University Science Books (1992),
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46 | ** section 2.553, p83. This contains references to
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47 | ** the Stephenson & Morrison and McCarthy & Babcock
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48 | ** papers.
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49 | **
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50 | ** Last revision: 14 February 1995
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51 | **
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52 | ** Copyright P.T.Wallace. All rights reserved.
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53 | */
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54 | {
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55 | double t, w, s;
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56 |
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57 |
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58 | /* Centuries since 1800 */
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59 | t = ( epoch - 1800.0 ) / 100.0;
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60 |
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61 | /* Select model */
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62 | if ( epoch >= 1708.185161980887 ) {
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63 |
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64 | /* Post-1708: use McCarthy & Babcock */
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65 | w = t - 0.19;
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66 | s = 5.156 + 13.3066 * w * w;
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67 | } else {
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68 | if ( epoch >= 979.0258204760233 ) {
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69 |
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70 | /* 979-1708: use Stephenson & Morrison's 948-1600 model */
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71 | s = 25.5 * t * t;
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72 | } else {
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73 |
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74 | /* Pre-979: use Stephenson & Morrison's 390 BC to AD 948 model */
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75 | s = 1360.0 + ( 320.0 + 44.3 * t ) * t;
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76 | }
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77 | }
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78 |
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79 | /* Result */
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80 | return s;
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81 | }
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