j1950_c |
Table of contents
Procedurej1950_c ( Julian Date of 1950.0 JAN 1.0 ) SpiceDouble j1950_c ( void ) AbstractReturn the Julian Date of 1950 JAN 01 00:00:00 (1950 JAN 1.0). Required_ReadingNone. KeywordsCONSTANTS Brief_I/OThe function returns the Julian Date of 1950 JAN 01 00:00:00 (1950 JAN 1.0). Detailed_InputNone. Detailed_OutputThe function returns 2433282.5, the Julian Date corresponding to 1950 JAN 01 00:00:00 (1950 JAN 1.0). ParametersNone. ExceptionsError free. FilesNone. ParticularsThe function always returns the constant value shown above. 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 J1950 date. Example code begins here. /. Program j1950_ex1 ./ #include <stdio.h> #include "SpiceUsr.h" int main( ) { /. Display the J1950 date in 16.8 floating point format ./ printf ( "J1950 date: %16.8f\n", j1950_c() ); return ( 0 ); } When this program was executed on a Mac/Intel/cc/64-bit platform, the output was: J1950 date: 2433282.50000000 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 j1950_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_ReferencesNone. Author_and_InstitutionJ. Diaz del Rio (ODC Space) W.L. Taber (JPL) I.M. Underwood (JPL) E.D. Wright (JPL) Version-CSPICE Version 1.0.1, 06-JUL-2021 (JDR) Edited the header to comply with NAIF standard. Added complete code examples. -CSPICE Version 1.0.0, 08-FEB-1998 (EDW) (WLT) (IMU) Index_Entriesjulian date of 1950.0 jan 1.0 |
Fri Dec 31 18:41:08 2021