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https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf19 Apr 2006: cos. ; ð13Þ. where apl=a, and fs;1, fd, and fi are coefficients corre-sponding to the secular, resonant direct, and resonant indi-rect parts of the disturbing function, respectively. ... The result is. cosm2 : 1. 0:39 0:061=e ; ð26Þ. and these lines -
THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...
https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf19 Apr 2006: a@ a(1 [ b)/[1 [ 2b(1 ] e cos f )/(1 [ e2)] , (19). ... e@ (1 [ b)1Je2 ] 2be cos f ] b2 , (20)u8 @ [ u8 f [ f @ arctan [b sin f/(b cos f ] e)]. -
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https://people.ast.cam.ac.uk/~wyatt/dgdj01.pdf19 Apr 2006: 0]B]B@uxG-N+?3TQGH+?IA-oxGH=?xRU>A]B@M1-N==?G4/2L<@Mr;T2R2]t+;-N=B+?G4x143]B=.-N2_3T"G4/"=?3]B@M/U-0/,y14@ ... GH141. Ây P. IpI. If. fp. Re(y) = I cos. Im(y) = I sin. {
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