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use Rem;
use crate;
use crateanp;
/// Earth rotation angle (IAU 2000 model).
///
/// This function is part of the International Astronomical Union's
/// SOFA (Standards of Fundamental Astronomy) software collection.
///
/// Status: canonical model.
///
/// Given:
/// ```
/// dj1,dj2 double UT1 as a 2-part Julian Date (see note)
/// ```
/// Returned (function value):
/// ```
/// double Earth rotation angle (radians), range 0-2pi
/// ```
/// Notes:
///
/// 1) The UT1 date dj1+dj2 is a Julian Date, apportioned in any
/// convenient way between the arguments dj1 and dj2. For example,
/// JD(UT1)=2450123.7 could be expressed in any of these ways,
/// among others:
/// ```
/// dj1 dj2
///
/// 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 and MJD methods are good compromises
/// between resolution and convenience. The date & time method is
/// best matched to the algorithm used: maximum precision is
/// delivered when the dj1 argument is for 0hrs UT1 on the day in
/// question and the dj2 argument lies in the range 0 to 1, or vice
/// versa.
///
/// 2) The algorithm is adapted from Expression 22 of Capitaine et al.
/// 2000. The time argument has been expressed in days directly,
/// and, to retain precision, integer contributions have been
/// eliminated. The same formulation is given in IERS Conventions
/// (2003), Chap. 5, Eq. 14.
///
/// Called:
/// ```
/// iauAnp normalize angle into range 0 to 2pi
/// ```
/// References:
///
/// Capitaine N., Guinot B. and McCarthy D.D, 2000, Astron.
/// Astrophys., 355, 398-405.
///
/// McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
/// IERS Technical Note No. 32, BKG (2004)