| 1 | #include "erfa.h"
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| 2 |
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| 3 | int eraUtctai(double utc1, double utc2, double *tai1, double *tai2)
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| 4 | /*
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| 5 | ** - - - - - - - - - -
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| 6 | ** e r a U t c t a i
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| 7 | ** - - - - - - - - - -
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| 8 | **
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| 9 | ** Time scale transformation: Coordinated Universal Time, UTC, to
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| 10 | ** International Atomic Time, TAI.
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| 11 | **
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| 12 | ** Given:
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| 13 | ** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-4)
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| 14 | **
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| 15 | ** Returned:
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| 16 | ** tai1,tai2 double TAI as a 2-part Julian Date (Note 5)
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| 17 | **
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| 18 | ** Returned (function value):
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| 19 | ** int status: +1 = dubious year (Note 3)
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| 20 | ** 0 = OK
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| 21 | ** -1 = unacceptable date
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| 22 | **
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| 23 | ** Notes:
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| 24 | **
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| 25 | ** 1) utc1+utc2 is quasi Julian Date (see Note 2), apportioned in any
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| 26 | ** convenient way between the two arguments, for example where utc1
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| 27 | ** is the Julian Day Number and utc2 is the fraction of a day.
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| 28 | **
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| 29 | ** 2) JD cannot unambiguously represent UTC during a leap second unless
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| 30 | ** special measures are taken. The convention in the present
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| 31 | ** function is that the JD day represents UTC days whether the
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| 32 | ** length is 86399, 86400 or 86401 SI seconds. In the 1960-1972 era
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| 33 | ** there were smaller jumps (in either direction) each time the
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| 34 | ** linear UTC(TAI) expression was changed, and these "mini-leaps"
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| 35 | ** are also included in the ERFA convention.
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| 36 | **
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| 37 | ** 3) The warning status "dubious year" flags UTCs that predate the
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| 38 | ** introduction of the time scale or that are too far in the future
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| 39 | ** to be trusted. See eraDat for further details.
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| 40 | **
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| 41 | ** 4) The function eraDtf2d converts from calendar date and time of day
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| 42 | ** into 2-part Julian Date, and in the case of UTC implements the
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| 43 | ** leap-second-ambiguity convention described above.
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| 44 | **
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| 45 | ** 5) The returned TAI1,TAI2 are such that their sum is the TAI Julian
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| 46 | ** Date.
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| 47 | **
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| 48 | ** Called:
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| 49 | ** eraJd2cal JD to Gregorian calendar
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| 50 | ** eraDat delta(AT) = TAI-UTC
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| 51 | ** eraCal2jd Gregorian calendar to JD
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| 52 | **
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| 53 | ** References:
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| 54 | **
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| 55 | ** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
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| 56 | ** IERS Technical Note No. 32, BKG (2004)
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| 57 | **
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| 58 | ** Explanatory Supplement to the Astronomical Almanac,
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| 59 | ** P. Kenneth Seidelmann (ed), University Science Books (1992)
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| 60 | **
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| 61 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 62 | ** Derived, with permission, from the SOFA library. See notes at end of file.
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| 63 | */
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| 64 | {
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| 65 | int big1;
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| 66 | int iy, im, id, j, iyt, imt, idt;
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| 67 | double u1, u2, fd, dat0, dat12, w, dat24, dlod, dleap, z1, z2, a2;
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| 68 |
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| 69 |
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| 70 | /* Put the two parts of the UTC into big-first order. */
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| 71 | big1 = ( utc1 >= utc2 );
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| 72 | if ( big1 ) {
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| 73 | u1 = utc1;
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| 74 | u2 = utc2;
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| 75 | } else {
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| 76 | u1 = utc2;
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| 77 | u2 = utc1;
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| 78 | }
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| 79 |
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| 80 | /* Get TAI-UTC at 0h today. */
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| 81 | j = eraJd2cal(u1, u2, &iy, &im, &id, &fd);
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| 82 | if ( j ) return j;
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| 83 | j = eraDat(iy, im, id, 0.0, &dat0);
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| 84 | if ( j < 0 ) return j;
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| 85 |
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| 86 | /* Get TAI-UTC at 12h today (to detect drift). */
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| 87 | j = eraDat(iy, im, id, 0.5, &dat12);
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| 88 | if ( j < 0 ) return j;
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| 89 |
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| 90 | /* Get TAI-UTC at 0h tomorrow (to detect jumps). */
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| 91 | j = eraJd2cal(u1+1.5, u2-fd, &iyt, &imt, &idt, &w);
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| 92 | if ( j ) return j;
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| 93 | j = eraDat(iyt, imt, idt, 0.0, &dat24);
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| 94 | if ( j < 0 ) return j;
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| 95 |
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| 96 | /* Separate TAI-UTC change into per-day (DLOD) and any jump (DLEAP). */
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| 97 | dlod = 2.0 * (dat12 - dat0);
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| 98 | dleap = dat24 - (dat0 + dlod);
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| 99 |
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| 100 | /* Remove any scaling applied to spread leap into preceding day. */
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| 101 | fd *= (ERFA_DAYSEC+dleap)/ERFA_DAYSEC;
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| 102 |
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| 103 | /* Scale from (pre-1972) UTC seconds to SI seconds. */
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| 104 | fd *= (ERFA_DAYSEC+dlod)/ERFA_DAYSEC;
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| 105 |
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| 106 | /* Today's calendar date to 2-part JD. */
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| 107 | if ( eraCal2jd(iy, im, id, &z1, &z2) ) return -1;
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| 108 |
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| 109 | /* Assemble the TAI result, preserving the UTC split and order. */
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| 110 | a2 = z1 - u1;
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| 111 | a2 += z2;
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| 112 | a2 += fd + dat0/ERFA_DAYSEC;
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| 113 | if ( big1 ) {
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| 114 | *tai1 = u1;
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| 115 | *tai2 = a2;
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| 116 | } else {
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| 117 | *tai1 = a2;
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| 118 | *tai2 = u1;
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| 119 | }
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| 120 |
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| 121 | /* Status. */
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| 122 | return j;
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| 123 |
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| 124 | }
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| 125 | /*----------------------------------------------------------------------
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| 126 | **
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| 127 | **
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| 128 | ** Copyright (C) 2013-2016, NumFOCUS Foundation.
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| 129 | ** All rights reserved.
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| 130 | **
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| 131 | ** This library is derived, with permission, from the International
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| 132 | ** Astronomical Union's "Standards of Fundamental Astronomy" library,
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| 133 | ** available from http://www.iausofa.org.
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| 134 | **
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| 135 | ** The ERFA version is intended to retain identical functionality to
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| 136 | ** the SOFA library, but made distinct through different function and
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| 137 | ** file names, as set out in the SOFA license conditions. The SOFA
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| 138 | ** original has a role as a reference standard for the IAU and IERS,
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| 139 | ** and consequently redistribution is permitted only in its unaltered
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| 140 | ** state. The ERFA version is not subject to this restriction and
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| 141 | ** therefore can be included in distributions which do not support the
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| 142 | ** concept of "read only" software.
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| 143 | **
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| 144 | ** Although the intent is to replicate the SOFA API (other than
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| 145 | ** replacement of prefix names) and results (with the exception of
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| 146 | ** bugs; any that are discovered will be fixed), SOFA is not
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| 147 | ** responsible for any errors found in this version of the library.
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| 148 | **
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| 149 | ** If you wish to acknowledge the SOFA heritage, please acknowledge
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| 150 | ** that you are using a library derived from SOFA, rather than SOFA
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| 151 | ** itself.
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| 152 | **
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| 153 | **
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| 154 | ** TERMS AND CONDITIONS
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| 155 | **
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| 156 | ** Redistribution and use in source and binary forms, with or without
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| 157 | ** modification, are permitted provided that the following conditions
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| 158 | ** are met:
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| 159 | **
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| 160 | ** 1 Redistributions of source code must retain the above copyright
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| 161 | ** notice, this list of conditions and the following disclaimer.
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| 162 | **
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| 163 | ** 2 Redistributions in binary form must reproduce the above copyright
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| 164 | ** notice, this list of conditions and the following disclaimer in
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| 165 | ** the documentation and/or other materials provided with the
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| 166 | ** distribution.
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| 167 | **
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| 168 | ** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
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| 169 | ** the International Astronomical Union nor the names of its
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| 170 | ** contributors may be used to endorse or promote products derived
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| 171 | ** from this software without specific prior written permission.
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| 172 | **
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| 173 | ** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
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| 174 | ** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
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| 175 | ** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
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| 176 | ** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
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| 177 | ** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
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| 178 | ** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
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| 179 | ** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
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| 180 | ** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
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| 181 | ** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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| 182 | ** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
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| 183 | ** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
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| 184 | ** POSSIBILITY OF SUCH DAMAGE.
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| 185 | **
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| 186 | */
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