b1900_c |
Table of contents
Procedureb1900_c ( Besselian Date 1900.0 ) SpiceDouble b1900_c ( void ) AbstractReturn the Julian Date corresponding to Besselian Date 1900.0. Required_ReadingNone. KeywordsCONSTANTS Brief_I/OThe function returns the Julian Date corresponding to Besselian date 1900.0. Detailed_InputNone. Detailed_OutputThe function returns 2415020.31352, the Julian Date corresponding to Besselian Date 1900.0 as reported by Lieske [1]. ParametersNone. ExceptionsError free. FilesNone. ParticularsLieske [1] defines a mapping from Julian Ephemeris Date to Besselian: BE = 1900. + (JED - 2415020.31352)/365.242198781 The inverse mapping being: JED = (BE - 1900.)*365.242198781 + 2415020.31352 ExamplesThe numerical results shown for these examples may differ across platforms. The results depend on the SPICE kernels used as input, the compiler and supporting libraries, and the machine specific arithmetic implementation. 1) Display the double precision value for the Julian Date corresponding to the Besselian date 1900.0. Example code begins here. /. Program b1900_ex1 ./ #include <stdio.h> #include "SpiceUsr.h" int main( ) { /. Display the B1900 date in 16.8 floating point format ./ printf ( "B1900 date: %16.8f\n", b1900_c() ); return ( 0 ); } When this program was executed on a Mac/Intel/cc/64-bit platform, the output was: B1900 date: 2415020.31352000 2) Convert an input time in UTC format to TDB seconds past the following reference epochs: - Besselian date 1900 and 1950; and - Julian date 1900, 1950, 2000 and 2100. Use the LSK kernel below to load the leap seconds and time constants required for the conversions. naif0012.tls Example code begins here. /. Program b1900_ex2 ./ #include <stdio.h> #include "SpiceUsr.h" int main( ) { /. Local constants. ./ #define UTCSTR "1991-NOV-26" /. Local variables. ./ SpiceDouble et; SpiceDouble jed; /. Load the LSK file. ./ furnsh_c ( "naif0012.tls" ); /. Convert input UTC string to Ephemeris Time. ./ str2et_c ( UTCSTR, &et ); printf ( "Input ephemeris time : %20.3f\n\n", et ); /. Convert the Ephemeris Time to Julian ephemeris date, i.e. Julian date relative to TDB time scale. ./ jed = unitim_c ( et, "ET", "JED" ); /. Convert Julian Date to TDB seconds past the reference epochs and output the results. ./ printf ( "TDB seconds past B1900: %20.3f\n", ( jed - b1900_c() ) * spd_c() ); printf ( "TDB seconds past B1950: %20.3f\n", ( jed - b1950_c() ) * spd_c() ); printf ( "TDB seconds past J1900: %20.3f\n", ( jed - j1900_c() ) * spd_c() ); printf ( "TDB seconds past J1950: %20.3f\n", ( jed - j1950_c() ) * spd_c() ); printf ( "TDB seconds past J2000: %20.3f\n", ( jed - j2000_c() ) * spd_c() ); printf ( "TDB seconds past J2100: %20.3f\n", ( jed - j2100_c() ) * spd_c() ); return ( 0 ); } When this program was executed on a Mac/Intel/cc/64-bit platform, the output was: Input ephemeris time : -255614341.817 TDB seconds past B1900: 2900118570.055 TDB seconds past B1950: 1322272271.321 TDB seconds past J1900: 2900145658.183 TDB seconds past J1950: 1322265658.183 TDB seconds past J2000: -255614341.817 TDB seconds past J2100: -3411374341.817 RestrictionsNone. Literature_References[1] J. Lieske, "Precession Matrix Based on IAU (1976) System of Astronomical Constants," Astron. Astrophys. 73, 282-284, 1979. Author_and_InstitutionJ. Diaz del Rio (ODC Space) W.L. Taber (JPL) I.M. Underwood (JPL) E.D. Wright (JPL) Version-CSPICE Version 1.1.1, 06-JUL-2021 (JDR) Edited the header to comply with NAIF standard. Added complete code examples. -CSPICE Version 1.1.0, 01-SEP-2005 (EDW) Added journal reference and associated citations. -CSPICE Version 1.0.1, 08-FEB-1998 (EDW) Corrected and clarified header entries. -CSPICE Version 1.0.0, 25-OCT-1997 (EDW) (WLT) (IMU) Index_Entriesbesselian date 1900.0 |
Fri Dec 31 18:41:01 2021