/rust/registry/src/index.crates.io-1949cf8c6b5b557f/sofars-0.6.1/src/fundargs/fapa03.rs
Line | Count | Source |
1 | | /// Fundamental argument, IERS Conventions (2003): |
2 | | /// general accumulated precession in longitude. |
3 | | /// |
4 | | /// Status: canonical model. |
5 | | /// |
6 | | /// Given: |
7 | | /// t f64 TDB, Julian centuries since J2000.0 (Note 1) |
8 | | /// |
9 | | /// Returned (function value): |
10 | | /// f64 general precession in longitude, radians (Note 2) |
11 | | /// |
12 | | /// Notes: |
13 | | /// |
14 | | /// 1) Though t is strictly TDB, it is usually more convenient to use |
15 | | /// TT, which makes no significant difference. |
16 | | /// |
17 | | /// 2) The expression used is as adopted in IERS Conventions (2003). It |
18 | | /// is taken from Kinoshita & Souchay (1990) and comes originally |
19 | | /// from Lieske et al. (1977). |
20 | | /// |
21 | | /// References: |
22 | | /// |
23 | | /// Kinoshita, H. and Souchay J. 1990, Celest.Mech. and Dyn.Astron. |
24 | | /// 48, 187 |
25 | | /// |
26 | | /// Lieske, J.H., Lederle, T., Fricke, W. & Morando, B. 1977, |
27 | | /// Astron.Astrophys. 58, 1-16 |
28 | | /// |
29 | | /// McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003), |
30 | | /// IERS Technical Note No. 32, BKG (2004) |
31 | 0 | pub fn fapa03(t: f64) -> f64 { |
32 | | /* General accumulated precession in longitude. */ |
33 | 0 | (0.02438175 + 0.00000538691 * t) * t |
34 | 0 | } |