EoM via Orbital Elements: Milankovitch elements Perturbed two-body dynamics: - x = [h]_e_L]TER' Assume Keplerian dynamics dominant, w/ small disturbing acceleration Gauss planetary equations 0 ཟ ad Є R3 x= f(x) + B(x)ad fo(x) = B(x) = (Vrh) μ 2.r -h T 0 h(h+z.h) r h 0:{ôm ông ôn h = ||h||2, r = ||r||2, 2 = [0, 0, 1]

EoM via Orbital Elements: Milankovitch elements Perturbed two-body dynamics: - x = [h]_e_L]TER' Assume Keplerian dynamics dominant, w/ small disturbing acceleration Gauss planetary equations 0 ཟ ad Є R3 x= f(x) + B(x)ad fo(x) = B(x) = (Vrh) μ 2.r -h T 0 h(h+z.h) r h 0:{ôm ông ôn h = ||h||2, r = ||r||2, 2 = [0, 0, 1]

Elements Of Electromagnetics

7th Edition

ISBN:9780190698614

Author:Sadiku, Matthew N. O.

Publisher:Sadiku, Matthew N. O.

ChapterMA: Math Assessment

Section: Chapter Questions

Problem 1.1MA

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