args[0]=message
args[1]=DB::DB::Message=HASH(0x309fba0)
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26.02.2008 15:50 | P. V. Artemii

Pishu diplom po morehodnoi astronomii, doshel do chasti gde neobhodimo napisat' samomu programmu dlya vychisleniya polozheniya planet (Venera, Mars, Yupiter, ,Saturn). No voznikla problema. V knige Miusa "Astronomicheskie algoritmy", est' vychisleniya geliocentricheskih shirot, dolgot i radius- vektorov planet. Tam imeetsya takaya formula: L = (L0 + L1*t +L2*t*t +L3*t*t*t +L4*t*t*t*t +L5*t*t*t*t*t)/100 000 000 (rad) V konce imeyutsya prilozheniya gde est' vse eti koefficienty (L0,L1,L2,L3,L4,L5), no ya ne mogu ponyat' po kakomu principu ih vybirat' i dlya chego daetsya formula L0=A*Cos(B+C*t) Tak ponimayu vse eti koef-ty podstavlyayutsya v formulu L0=A*Cos(B+C*t) t.e.: L0=1.0564 *cos(3.6933+89624555.3*t) +1803.0*cos(4.1033+5661.3320*t) +........ i t.d Eto tak?

• >> Pomogite ili ob'yasnite.   (P. V. Artemii, 26.02.2008 15:50, 775 Bait)