pmat06¶
- erfa.pmat06(date1, date2)[source]¶
Precession matrix (including frame bias) from GCRS to a specified date, IAU 2006 model.
- Parameters:
- date1double array
- date2double array
- Returns:
- rbpdouble array
Notes
Wraps ERFA function
eraPmat06
. The ERFA documentation is:- - - - - - - - - - e r a P m a t 0 6 - - - - - - - - - - Precession matrix (including frame bias) from GCRS to a specified date, IAU 2006 model. Given: date1,date2 double TT as a 2-part Julian Date (Note 1) Returned: rbp double[3][3] bias-precession matrix (Note 2) Notes: 1) The TT date date1+date2 is a Julian Date, apportioned in any convenient way between the two arguments. For example, JD(TT)=2450123.7 could be expressed in any of these ways, among others: date1 date2 2450123.7 0.0 (JD method) 2451545.0 -1421.3 (J2000 method) 2400000.5 50123.2 (MJD method) 2450123.5 0.2 (date & time method) The JD method is the most natural and convenient to use in cases where the loss of several decimal digits of resolution is acceptable. The J2000 method is best matched to the way the argument is handled internally and will deliver the optimum resolution. The MJD method and the date & time methods are both good compromises between resolution and convenience. 2) The matrix operates in the sense V(date) = rbp * V(GCRS), where the p-vector V(GCRS) is with respect to the Geocentric Celestial Reference System (IAU, 2000) and the p-vector V(date) is with respect to the mean equatorial triad of the given date. Called: eraPfw06 bias-precession F-W angles, IAU 2006 eraFw2m F-W angles to r-matrix References: Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855 IAU: Trans. International Astronomical Union, Vol. XXIVB; Proc. 24th General Assembly, Manchester, UK. Resolutions B1.3, B1.6. (2000) Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981 This revision: 2021 May 11 Copyright (C) 2013-2023, NumFOCUS Foundation. Derived, with permission, from the SOFA library. See notes at end of file.