2011
DOI: 10.5028/jatm.2011.03032011
|View full text |Cite
|
Sign up to set email alerts
|

15:1 Resonance effects on the orbital motion of artificial satellites

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
2
0

Year Published

2013
2013
2023
2023

Publication Types

Select...
4
1
1

Relationship

0
6

Authors

Journals

citations
Cited by 9 publications
(2 citation statements)
references
References 9 publications
(4 reference statements)
0
2
0
Order By: Relevance
“…Kuznetsov (2010) [14] discussed the properties of resonance zones and analyzed them as a function of the semi-major axes using the Hori-DePrit method. Formiga and Moraes (2011) [7] have discussed the motion of artificial satellites on 15:1 resonance under the impact of geopotential perturbations.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Kuznetsov (2010) [14] discussed the properties of resonance zones and analyzed them as a function of the semi-major axes using the Hori-DePrit method. Formiga and Moraes (2011) [7] have discussed the motion of artificial satellites on 15:1 resonance under the impact of geopotential perturbations.…”
Section: Introductionmentioning
confidence: 99%
“…, (4),(5), and (6) are represent the 2-D resonant curves at the resonant points θm0 = 2 γ, 3 θm0 = 2 γ, θm0 = γ, θm0 = α0 , and 3 θm0 = 2 α0 for amplitudes A (b)1 , A (b)3 , A (b)5 and A (b)6 for the suitability of coefficient of resistive force (b). We have observed that the Moon's motion has zerodamping, light damping, medium damping, and heavy damping for the values b = 0, 0.1, 0.2, 0.3.• In figure(7), we have studied the impact of eccentricity (e) on the amplitudes A (b)1 , A (b)3 , A (b)5 , and A (b)6 . In this case, figures represents that the amplitudes increase when eccentricity increases.• In figure(8), we have analyzed the impact of semi-major axis (a) on amplitudes A (b)1 , A (b)3 , A (b)5 , and A (b)6 .…”
mentioning
confidence: 99%