uddc_c |
Table of contents
Procedureuddc_c ( Derivative of function less than zero, df(x)/dx < 0 ) void uddc_c ( void ( * udfunc ) ( SpiceDouble x, SpiceDouble * value ), SpiceDouble x, SpiceDouble dx, SpiceBoolean * isdecr ) AbstractReturn SPICETRUE if the derivative of the callback function `udfunc' at a given abscissa value is negative. Required_ReadingGF KeywordsDERIVATIVE GEOMETRY Brief_I/OVARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- udfunc I The routine that computes the scalar value of interest. x I Independent variable of 'udfunc'. dx I Interval from 'x' for derivative calculation. isdecr O Boolean indicating if the derivative is negative. Detailed_Inputudfunc is the routine that returns the value of the scalar quantity function of interest at `x'. The calling sequence for `udfunc' is: udfunc ( x, &value ); where: x is the double precision value of the independent variable of the function at which to determine the scalar value. value is the double precision value returned by `udfunc' at `x'. Functionally: value = udfunc ( x ) x is a scalar double precision value at which to determine the derivative of `udfunc'. For many SPICE uses, `x' will represent ephemeris time, expressed as seconds past J2000 TDB. dx is a scalar double precision value representing half the interval in units of `x' separating the evaluation values of `udfunc'; the evaluations occur at (x + dx) and (x - dx). `dx' may be negative but must be non-zero. Detailed_Outputisdecr is a scalar boolean indicating if the first derivative of `udfunc' with respect to time at `et' is less than zero. Functionally: d udfunc(x) | ----------- | < 0 dx | x ParametersNone. Exceptions1) If `dx' has a value of zero, an error is signaled by a routine in the call tree of this routine. FilesIf the evaluation of 'udfunc' requires SPICE kernel data, the appropriate kernels must be loaded before calling this routine. - SPK data: the calling application must load ephemeris data for the targets, observer, and any intermediate objects in a chain connecting the targets and observer for the time used in the evaluation. If aberration corrections are used, the states of target and observer relative to the solar system barycenter must be calculable from the available ephemeris data. - If non-inertial reference frames are used, then PCK files, frame kernels, C-kernels, and SCLK kernels may be needed. Such kernel data are normally loaded once per program run, NOT every time this routine is called. ParticularsNone. ExamplesSee gfuds_c. RestrictionsNone. Literature_ReferencesNone. Author_and_InstitutionN.J. Bachman (JPL) J. Diaz del Rio (ODC Space) E.D. Wright (JPL) Version-CSPICE Version 1.0.1, 01-NOV-2021 (JDR) Edited the header to comply with NAIF standard. -CSPICE Version 1.0.0, 31-MAR-2010 (EDW) (NJB) Index_Entriesfirst derivative less-than zero |
Fri Dec 31 18:41:14 2021