Satellite orbit decay due to atmospheric drag

Author(s):  
Y. Kim ◽  
G. Vukovich
1966 ◽  
Author(s):  
C. GAZLEY ◽  
L. ROWELL ◽  
G. SCHILLING
Keyword(s):  

2010 ◽  
Vol 410 (1) ◽  
pp. 654-662 ◽  
Author(s):  
Guochang Xu ◽  
Xu Tianhe ◽  
Wu Chen ◽  
Ta-Kang Yeh

2020 ◽  
Vol 8 (1) ◽  
pp. 19
Author(s):  
T. R. Saritha Kumari ◽  
M. Xavier James Raj

Satellite moving under the gravitational field of Earth deviates from its two-body elliptic orbit, due to the combined effects of the gravitational field of Earth, atmospheric drag, solar radiation pressure, third-body gravitational effects, etc. This paper utilizes the KS regular element equations to solve Newtonian equations of motion to obtain numerical solution with respect to perturbing forces, like, Earth's gravity (includes zonal, sectorial and tesseral harmonics terms), atmospheric drag and solar radiation pressure. Effectiveness of the theory is illustrated by comparing the results with some of the existing theories in literature. 


Author(s):  
Ehsan Taheri ◽  
Robert A. Zidek ◽  
Ilya Kolmanovsky ◽  
Anouck Girard

2017 ◽  
pp. 53-58 ◽  
Author(s):  
M.M. Martinovic ◽  
S.D. Segan

The report studies some changes in orbital elements of the artificial satellites of Earth under influence of atmospheric drag. In order to develop possibilities of applying the results in many future cases, an analytical interpretation of the orbital element perturbations is given via useful, but very long expressions. The development is based on the TD88 air density model, recently upgraded with some additional terms. Some expressions and formulae were developed by the computer algebra system Mathematica and tested in some hypothetical cases. The results have good agreement with iterative (numerical) approach.


1966 ◽  
Vol 25 ◽  
pp. 363-371
Author(s):  
P. Sconzo

In this paper an orbit computation program for artificial satellites is presented. This program is operational and it has already been used to compute the orbits of several satellites.After an introductory discussion on the subject of artificial satellite orbit computations, the features of this program are thoroughly explained. In order to achieve the representation of the orbital elements over short intervals of time a drag-free perturbation theory coupled with a differential correction procedure is used, while the long range behavior is obtained empirically. The empirical treatment of the non-gravitational effects upon the satellite motion seems to be very satisfactory. Numerical analysis procedures supporting this treatment and experience gained in using our program are also objects of discussion.


2015 ◽  
Vol 8 (5) ◽  
pp. 174
Author(s):  
Ayman Hamdy Kassem ◽  
Gamal Mohamad El-Bayoumi ◽  
Tamer Mekky Habib ◽  
Karim Ahmed Kamalaldin

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