Calculate the (cross-)power spectrum expectation of a windowed function from its global spectrum.
Usage
call SHBias (shh
, lwin
, incspectra
, ldata
, outcspectra
, save_cg
, exitstatus
)
Parameters
shh
: input, real(dp), dimension (lwin
+1)- The power spectrum of the localizing window.
lwin
: input, integer(int32)- The spherical harmonic bandwidth of the localizing window.
incspectra
: input, real(dp), dimension (ldata
+1)- The global unwindowed (cross-)power spectrum.
ldata
: input, integer(int32)- The maximum degree of the global unwindowed power spectrum.
outcspectra
: output, real(dp), dimension (ldata
+lwin
+1)- The expectation of the localized (cross-)power spectrum.
save_cg
: optional, input, integer(int32), default = 0- If set equal to 1, the Clebsch-Gordon coefficients will be precomputed and saved for future use (if
lwin
orldata
change, this will be recomputed). To deallocate the saved memory, set this parameter equal to -1. If set equal to 0 (default), the Clebsch-Gordon coefficients will be recomputed for each call. exitstatus
: output, optional(int32), integer- If present, instead of executing a STOP when an error is encountered, the variable exitstatus will be returned describing the error. 0 = No errors; 1 = Improper dimensions of input array; 2 = Improper bounds for input variable; 3 = Error allocating memory; 4 = File IO error.
Description
SHBias
will calculate the (cross-)power spectrum expectation of a function multiplied by a localizing window. This is given by equation 35 of Wieczorek and Simons (2005) and equation 2.11 of Wieczorek and Simons (2007),
<SFG> = Sum_{j=0}^L Shh Sum_{i=|l-j|}^{|l+j|} Sfg (C_{j0i0}^{l0})^2
where <SFG>
is the expectation of the localized (cross-)power spectrum, Shh
is the power spectrum of the window bandlimited to degree L
, Sfg
is the global unwindowed (cross-)power spectrum, and C
is a Clebsch-Gordan coefficient. The Clebsch-Gordan coefficients are calculated using a simple relationship to the Wigner 3-j symbols. The maximum calculated degree of the windowed power spectrum expectation corresponds to the smaller of (ldata+lwin
) and size(outcspectra)-1
. It is implicitly assumed that the power spectrum of inspectrum
is zero beyond degree ldata.
. If this is not the case, the ouput power spectrum should be considered valid only for the degrees up to and including ldata
- lwin
.
If this routine is to be called several times using the same values of lwin
and ldata
, then the Clebsch-Gordon coefficients can be precomputed and saved by setting the optional parameter save_cg
equal to 1. To deallocate the saved memory, which is a matrix of size (lwin+ldata,lwin,2*lwin+ldata+1
), set save_cg
equal to -1.
References
Wieczorek, M. A. and F. J. Simons, Localized spectral analysis on the sphere, Geophys. J. Int., 162, 655-675, doi:10.1111/j.1365-246X.2005.02687.x, 2005.
Wieczorek, M. A. and F. J. Simons, Minimum-variance multitaper spectral estimation on a sphere, J. Fourier Anal. Appl., 13, 665-692, doi:10.1007/s00041-006-6904-1, 2007.
See also
shpowerspectrum,shcrosspowerspectrum, wigner3j, shreturntapers, shreturntapersm, shbiasadmitcorr
Edit me