2017
DOI: 10.1016/j.jappmathmech.2017.08.002
|View full text |Cite
|
Sign up to set email alerts
|

Stability of the steady rotations of a satellite with internal damping in a central gravitational field

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

0
21
0

Year Published

2017
2017
2024
2024

Publication Types

Select...
3
2
1

Relationship

0
6

Authors

Journals

citations
Cited by 13 publications
(21 citation statements)
references
References 4 publications
0
21
0
Order By: Relevance
“…Based on the Eqs. (36a) -(36d) and the particular solutions (28) and (30), if γ * = 3, q * 1 = ν/2, the unperturbed motion (37) and the Hamiltonian (39) corresponding to the particular solution (28); if γ * = 1, q * 1 = −ν/2, they corresponding to another particular solution (30). According to the Eq.…”
Section: Particular Solutions and The Equations Of Perturbed Motionmentioning
confidence: 99%
See 4 more Smart Citations
“…Based on the Eqs. (36a) -(36d) and the particular solutions (28) and (30), if γ * = 3, q * 1 = ν/2, the unperturbed motion (37) and the Hamiltonian (39) corresponding to the particular solution (28); if γ * = 1, q * 1 = −ν/2, they corresponding to another particular solution (30). According to the Eq.…”
Section: Particular Solutions and The Equations Of Perturbed Motionmentioning
confidence: 99%
“…According to the Eqs. (43) and (44), the necessary conditions for the existence of the particular solutions (28) and (30) are given as follows:…”
Section: Particular Solutions and The Equations Of Perturbed Motionmentioning
confidence: 99%
See 3 more Smart Citations