1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
use pn00b;
/// Form the matrix of nutation for a given date, IAU 2000B model.
///
/// This function is part of the International Astronomical Union's
/// SOFA (Standards of Fundamental Astronomy) software collection.
///
/// Status: support function.
///
/// Given:
/// date1,date2 double TT as a 2-part Julian Date (Note 1)
///
/// Returned (function value):
/// rmatn [[f64; 3]; 3] nutation matrix
///
/// 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(true) = rmatn * V(mean), where
/// the p-vector V(true) is with respect to the true equatorial triad
/// of date and the p-vector V(mean) is with respect to the mean
/// equatorial triad of date.
///
/// 3) The present function is faster, but slightly less accurate (about
/// 1 mas), than the iauNum00a function.
///
/// Called:
/// iauPn00b bias/precession/nutation, IAU 2000B
///
/// Reference:
///
/// Explanatory Supplement to the Astronomical Almanac,
/// P. Kenneth Seidelmann (ed), University Science Books (1992),
/// Section 3.222-3 (p114).