rfa 0.5.9

A port ERFA to Rust.
Documentation
use crate::rfam::*;
///  Precession-rate part of the IAU 2000 precession-nutation models
///  (part of MHB2000).
///
///  Given:
///   * date1,date2 TT as a 2-part Julian Date (Note 1)
///
///  Returned:
///   * dpsipr,depspr precession corrections (Notes 2,3)
///
/// # 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 precession adjustments are expressed as "nutation
///     components", corrections in longitude and obliquity with respect
///     to the J2000.0 equinox and ecliptic.
///
///  3) Although the precession adjustments are stated to be with respect
///     to Lieske et al. (1977), the MHB2000 model does not specify which
///     set of Euler angles are to be used and how the adjustments are to
///     be applied.  The most literal and straightforward procedure is to
///     adopt the 4-rotation epsilon_0, psi_A, omega_A, xi_A option, and
///     to add dpsipr to psi_A and depspr to both omega_A and eps_A.
///
///  4) This is an implementation of one aspect of the IAU 2000A nutation
///     model, formally adopted by the IAU General Assembly in 2000,
///     namely MHB2000 (Mathews et al. 2002).
///
/// # References:
///   * Lieske, J.H., Lederle, T., Fricke, W. & Morando, B., "Expressions
///     for the precession quantities based upon the IAU (1976) System of
///     Astronomical Constants", Astron.Astrophys., 58, 1-16 (1977)
///   * Mathews, P.M., Herring, T.A., Buffet, B.A., "Modeling of nutation
///     and precession   New nutation series for nonrigid Earth and
///     insights into the Earth's interior", J.Geophys.Res., 107, B4,
///     2002.  The MHB2000 code itself was obtained on 9th September 2002
///     from ftp://maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
///   * Wallace, P.T., "Software for Implementing the IAU 2000
///     Resolutions", in IERS Workshop 5.1 (2002).
///
///  This revision:  2021 May 11
pub fn pr00(date1: f64, date2: f64, dpsipr: &mut f64, depspr: &mut f64)
{

/* Precession and obliquity corrections (radians per century) */
    const PRECOR: f64 = -0.29965 * URSA_DAS2R;
    const OBLCOR: f64 = -0.02524 * URSA_DAS2R;


/* Interval between fundamental epoch J2000.0 and given date (JC). */
   let t = ((date1 - URSA_DJ00) + date2) / URSA_DJC;

/* Precession rate contributions with respect to IAU 1976/80. */
   *dpsipr = PRECOR * t;
   *depspr = OBLCOR * t;

/* Finished. */

}