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legendreprodintRadLatvar.m
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legendreprodintRadLatvar.m
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function varargout=legendreprodintRadLatvar(L1,m1,L2,m2,x0,method,rplanet,rsatfun)
% in=legendreprodintRadLatvar(L1,m1,L2,m2,x0,method,rplanet,rsatfun)
%
% This function is designed for the radial derivative of the potential
% field at satellite altitude with a satellite radial position that
% varies with latitude, given as a function handle rsatfun
%
% Evaluates the integral of the product of two Schmidt semi-normalized
% real Legendre polynomials P_lm(x)P_l'm'(x)dx from x to 1, where that
% means using Matlab's LEGENDRE([],[],'sch'), see XLM, YLM, PLM etc.
%
%
% The normalization is such that the integration amounts to
% (4-2*(m==0))/(2l+1) over the entire interval from -1 to 1,
% This normalizes the spherical harmonics to 4\pi/(2l+1).
% Note Schmidt contains the sqrt(2) multiplying Xlm.
%
% INPUT:
%
% L1,L2 Angular degrees of the polynomials, L1,L2>=0
% m1,m2 Angular orders of the polynomials, 0<=m<=L
% x0 Single point with lower integration limit
% method 'automatic' Using analytical formula if possible (default)
% 'dumb' Forcing usage of dumb semi-analytical formula
% 'gl' Exact result by Gauss-Legendre integration, when m1~=m2
% 'paul' By Wigner expansion and the method of Paul (1978)
% rplanet planetary radial position
% rsatfun function handle for satellite radial position depending
% on sin(latitude) or cos(colatitude)
% savename unique name you want to use for this function handle to
% save and restore the calculated kernels
%
%
% OUTPUT:
%
% in The integrated product.
%
% EXAMPLE:
%
% legendreprodint('demo1') Wigner recursion vs. Gauss-Legendre, L1=L2, m=0
% legendreprodint('demo2') Wigner recursion vs. Gauss-Legendre, L1~=L2, m=0
% legendreprodint('demo3') Dumb summation vs. Gauss-Legendre, L1=L2, m=0
% legendreprodint('demo4') Paul recursion vs. Gauss-Legendre
% legendreprodint('demo5') Verify some analytical formulas
%
% Original by
% Last modified by plattner-at-princeton.edu, 05/24/2011
% Last modified by fjsimons-at-alum.mit.edu, 06/12/2015
%
% Last modified by plattner-at-alumni.ethz.ch, 7/12/2018
if ~isstr(L1)
defval('L1',1)
defval('m1',0)
defval('L2',2)
defval('m2',0)
defval('x0',0)
defval('method','automatic')
if length(x0)~=1 && ~strcmp(method,'paul')
error('Not for multiple limits')
end
% Standard spherical harmonics restrictions using LEGENDRE or LIBBRECHT
if m1>L1 | m2>L2 | m1<0 | m2<0
error('Positive order must be smaller or equal than degree')
end
% If 'gl' requested by the user or required by the problem
% Using Gauss-Legendre integration from
% http://mathworld.wolfram.com/Legendre-GaussQuadrature.html
% Formulate the integrand as an inline function, anonymous is better
integrand=inline(sprintf(...
['rindeks(repmat((-%i-1)/%g*(%s(x)/%g).^(-%i-2),%i+1,1).*legendre(%i,x,''sch''),%i).*',...
'rindeks(repmat((-%i-1)/%g*(%s(x)/%g).^(-%i-2),%i+1,1).*legendre(%i,x,''sch''),%i)'],...
L1,rplanet,func2str(rsatfun),rplanet,L1,L1,L1,m1+1,...
L2,rplanet,func2str(rsatfun),rplanet,L2,L2,L2,m2+1));
% Calculate the Gauss-Legendre coefficients
% Watch out: multiply if m is not 0
[w,xgl,nsel]=gausslegendrecof(max(L1+L2,...
max(200*((m1*m2)~=0),...
1000*mod(m1+m2,2))));
% For l=1 and m=0 this is not even close to enough nodes
% Calculate integral
in=gausslegendre([x0 1],integrand,[w(:) xgl(:)]);
% disp(sprintf('Gauss-Legendre with %i points',nsel))
end
varns={in};
varargout=varns(1:nargout);