public class PoissonSeriesParser extends Object
Poisson series
files.
A Poisson series is composed of a time polynomial part and a non-polynomial
part which consist in summation series. The series terms
are harmonic functions (combination of sines and cosines) of polynomial
arguments. The polynomial arguments are combinations of luni-solar or
planetary elements
.
The Poisson series files from IERS have various formats, with or without polynomial part, with or without planetary components, with or without period column, with terms of increasing degrees either in dedicated columns or in successive sections of the file ... This class attempts to read all the commonly found formats, by specifying the columns of interest.
The handling of increasing degrees terms (i.e. sin, cos, t sin, t cos, t^2 sin, t^2 cos ...) is done as follows.
A file from an old convention, like table 5.1 in IERS conventions 1996, uses separate columns for degree 0 and degree 1, and uses only sine for nutation in longitude and cosine for nutation in obliquity. It reads as follows:
∆ψ = Σ (Ai+A'it) sin(ARGUMENT), ∆ε = Σ (Bi+B'it) cos(ARGUMENT) MULTIPLIERS OF PERIOD LONGITUDE OBLIQUITY l l' F D Om days Ai A'i Bi B'i 0 0 0 0 1 -6798.4 -171996 -174.2 92025 8.9 0 0 2 -2 2 182.6 -13187 -1.6 5736 -3.1 0 0 2 0 2 13.7 -2274 -0.2 977 -0.5 0 0 0 0 2 -3399.2 2062 0.2 -895 0.5
In order to parse the nutation in longitude from the previous table, the following settings should be used:
PoissonSeriesParser(int)
)withFirstDelaunay(int)
)withFirstPlanetary(int)
as there are no planetary columns in this tablewithSinCos(int, int, double, int, double)
)withSinCos(int, int, double, int, double)
)In order to parse the nutation in obliquity from the previous table, the following settings should be used:
PoissonSeriesParser(int)
)withFirstDelaunay(int)
)withFirstPlanetary(int)
as there are no planetary columns in this tablewithSinCos(int, int, double, int, double)
)withSinCos(int, int, double, int, double)
)A file from a recent convention, like table 5.3a in IERS conventions 2010, uses only two columns for sin and cos, and separate degrees in successive sections with dedicated headers. It reads as follows:
--------------------------------------------------------------------------------------------------- (unit microarcsecond; cut-off: 0.1 microarcsecond) (ARG being for various combination of the fundamental arguments of the nutation theory) Sum_i[A_i * sin(ARG) + A"_i * cos(ARG)] + Sum_i[A'_i * sin(ARG) + A"'_i * cos(ARG)] * t (see Chapter 5, Eq. (35)) The Table below provides the values for A_i and A"_i (j=0) and then A'_i and A"'_i (j=1) The expressions for the fundamental arguments appearing in columns 4 to 8 (luni-solar part) and in columns 9 to 17 (planetary part) are those of the IERS Conventions 2003 ---------------------------------------------------------------------------------------------------------- j = 0 Number of terms = 1320 ---------------------------------------------------------------------------------------------------------- i A_i A"_i l l' F D Om L_Me L_Ve L_E L_Ma L_J L_Sa L_U L_Ne p_A ---------------------------------------------------------------------------------------------------------- 1 -17206424.18 3338.60 0 0 0 0 1 0 0 0 0 0 0 0 0 0 2 -1317091.22 -1369.60 0 0 2 -2 2 0 0 0 0 0 0 0 0 0 3 -227641.81 279.60 0 0 2 0 2 0 0 0 0 0 0 0 0 0 4 207455.40 -69.80 0 0 0 0 2 0 0 0 0 0 0 0 0 0 5 147587.70 1181.70 0 1 0 0 0 0 0 0 0 0 0 0 0 0 ... 1319 -0.10 0.00 0 0 0 0 0 1 0 -3 0 0 0 0 0 -2 1320 -0.10 0.00 0 0 0 0 0 0 0 1 0 1 -2 0 0 0 -------------------------------------------------------------------------------------------------------------- j = 1 Number of terms = 38 -------------------------------------------------------------------------------------------------------------- i A'_i A"'_i l l' F D Om L_Me L_Ve L_E L_Ma L_J L_Sa L_U L_Ne p_A -------------------------------------------------------------------------------------------------------------- 1321 -17418.82 2.89 0 0 0 0 1 0 0 0 0 0 0 0 0 0 1322 -363.71 -1.50 0 1 0 0 0 0 0 0 0 0 0 0 0 0 1323 -163.84 1.20 0 0 2 -2 2 0 0 0 0 0 0 0 0 0 1324 122.74 0.20 0 1 2 -2 2 0 0 0 0 0 0 0 0 0
In order to parse the nutation in longitude from the previous table, the following settings should be used:
PoissonSeriesParser(int)
)withFirstDelaunay(int)
)withFirstPlanetary(int)
)withSinCos(int, int, double, int, double)
...)
A file from a recent convention, like table 6.5a in IERS conventions 2010, contains
both Doodson arguments (τ, s, h, p, N', ps), Doodson numbers and Delaunay parameters.
In this case, the coefficients for the Delaunay parameters must be subtracted
from the τ = GMST + π tide parameter, so the signs in the files must be reversed
in order to match the Doodson arguments and Doodson numbers. This is done automatically
(and consistency is checked) only when the withDoodson(int, int)
method is
called at parser configuration time. Some other files use the γ = GMST + π tide parameter
rather than Doodson τ argument and the coefficients for the Delaunay parameters must be
added to the γ parameter, so no sign reversal is performed. In order to avoid
ambiguity as the two cases are incompatible with each other, trying to add a configuration
for τ by calling withDoodson(int, int)
and to also add a configuration for γ by
calling withGamma(int)
triggers an exception.
The table 6.5a file also contains a column for the waves names (the Darwin's symbol)
which may be empty, so it must be identified explicitly by calling withOptionalColumn(int)
. The 6.5a table reads as follows:
The in-phase (ip) amplitudes (A₁ δkfR Hf) and the out-of-phase (op) amplitudes (A₁ δkfI Hf) of the corrections for frequency dependence of k₂₁⁽⁰⁾, taking the nominal value k₂₁ for the diurnal tides as (0.29830 − i 0.00144). Units: 10⁻¹² . The entries for δkfR and δkfI are in units of 10⁻⁵. Multipliers of the Doodson arguments identifying the tidal terms are given, as also those of the Delaunay variables characterizing the nutations produced by these terms. Name deg/hr Doodson τ s h p N' ps l l' F D Ω δkfR δkfI Amp. Amp. No. /10−5 /10−5 (ip) (op) 2Q₁ 12.85429 125,755 1 -3 0 2 0 0 2 0 2 0 2 -29 3 -0.1 0.0 σ₁ 12.92714 127,555 1 -3 2 0 0 0 0 0 2 2 2 -30 3 -0.1 0.0 13.39645 135,645 1 -2 0 1 -1 0 1 0 2 0 1 -45 5 -0.1 0.0 Q₁ 13.39866 135,655 1 -2 0 1 0 0 1 0 2 0 2 -46 5 -0.7 0.1 ρ₁ 13.47151 137,455 1 -2 2 -1 0 0 -1 0 2 2 2 -49 5 -0.1 0.0
PoissonSeriesParser(int)
)withOptionalColumn(int)
)withDoodson(int, int)
)withFirstDelaunay(int)
)withSinCos(int, int, double, int, double)
...)Our parsing algorithm involves adding the section degree from the "j = 0, 1, 2 ..." header to the column degree. A side effect of this algorithm is that it is theoretically possible to mix both formats and have for example degree two term appear as degree 2 column in section j=0 and as degree 1 column in section j=1 and as degree 0 column in section j=2. This case is not expected to be encountered in practice. The real files use either several columns or several sections, but not both at the same time.
SeriesTerm
,
PolynomialNutation
Constructor and Description |
---|
PoissonSeriesParser(int totalColumns)
Build a parser for a Poisson series from an IERS table file.
|
Modifier and Type | Method and Description |
---|---|
PoissonSeries |
parse(InputStream stream,
String name)
Parse a stream.
|
PoissonSeriesParser |
withDoodson(int firstMultiplierColumn,
int numberColumn)
Set up columns for Doodson multipliers and Doodson number.
|
PoissonSeriesParser |
withFirstDelaunay(int firstColumn)
Set up first column of Delaunay multiplier.
|
PoissonSeriesParser |
withFirstPlanetary(int firstColumn)
Set up first column of planetary multiplier.
|
PoissonSeriesParser |
withGamma(int column)
Set up column of GMST tide multiplier.
|
PoissonSeriesParser |
withOptionalColumn(int column)
Set up optional column.
|
PoissonSeriesParser |
withPolynomialPart(char freeVariable,
PolynomialParser.Unit unit)
Set up polynomial part parsing.
|
PoissonSeriesParser |
withSinCos(int degree,
int sinColumn,
double sinFactor,
int cosColumn,
double cosFactor)
Set up columns of the sine and cosine coefficients.
|
public PoissonSeriesParser(int totalColumns)
totalColumns
- total number of columns in the non-polynomial sectionspublic PoissonSeriesParser withPolynomialPart(char freeVariable, PolynomialParser.Unit unit)
freeVariable
- name of the free variable in the polynomial partunit
- default unit for polynomial, if not explicit within the filepublic PoissonSeriesParser withOptionalColumn(int column)
Optional columns typically appears in tides-related files, as some waves have specific names (χ₁, M₂, ...) and other waves don't have names and hence are replaced by spaces in the corresponding file line.
At most one column may be optional.
column
- optional column (counting from 1)public PoissonSeriesParser withGamma(int column)
column
- column of the GMST tide multiplier (counting from 1)withDoodson(int, int)
public PoissonSeriesParser withDoodson(int firstMultiplierColumn, int numberColumn)
firstMultiplierColumn
- column of the first Doodson multiplier which
corresponds to τ (counting from 1)numberColumn
- column of the Doodson number (counting from 1)withGamma(int)
,
withFirstDelaunay(int)
public PoissonSeriesParser withFirstDelaunay(int firstColumn)
firstColumn
- column of the first Delaunay multiplier (counting from 1)public PoissonSeriesParser withFirstPlanetary(int firstColumn)
firstColumn
- column of the first planetary multiplier (counting from 1)public PoissonSeriesParser withSinCos(int degree, int sinColumn, double sinFactor, int cosColumn, double cosFactor)
degree
- degree to set upsinColumn
- column of the sine coefficient for tdegree counting from 1
(may be -1 if there are no sine coefficients)sinFactor
- multiplicative factor for the sine coefficientcosColumn
- column of the cosine coefficient for tdegree counting from 1
(may be -1 if there are no cosine coefficients)cosFactor
- multiplicative factor for the cosine coefficientpublic PoissonSeries parse(InputStream stream, String name)
stream
- stream containing the IERS tablename
- name of the resource file (for error messages only)Copyright © 2002-2022 CS GROUP. All rights reserved.