Variation of Earth's Oblateness J 2 on Interannual‐to‐Decadal Timescales

Author(s):  
B. F. Chao ◽  
Y. Yu ◽  
C. H. Chung
Keyword(s):  
1956 ◽  
Vol 27 (10) ◽  
pp. 1141-1149 ◽  
Author(s):  
Leon Blitzer ◽  
Morris Weisfeld ◽  
Albert D. Wheelon
Keyword(s):  

2019 ◽  
Vol 46 (1) ◽  
pp. 158-168 ◽  
Author(s):  
Yu Sun ◽  
Riccardo Riva ◽  
Pavel Ditmar ◽  
Roelof Rietbroek
Keyword(s):  

1993 ◽  
Vol 13 (8) ◽  
pp. 171-174 ◽  
Author(s):  
J. Ashenberg ◽  
R.A. Broucke
Keyword(s):  

2004 ◽  
Vol 109 (B9) ◽  
pp. n/a-n/a ◽  
Author(s):  
Minkang Cheng ◽  
Byron D. Tapley

2013 ◽  
Vol 2013 ◽  
pp. 1-11 ◽  
Author(s):  
Iván Pérez ◽  
Juan Félix San-Juan ◽  
Montserrat San-Martín ◽  
Luis María López-Ochoa

We present a new approach in astrodynamics and celestial mechanics fields, calledhybrid perturbation theory. A hybrid perturbation theory combines anintegrating technique, general perturbation theory or special perturbation theory or semianalytical method, with aforecasting technique, statistical time series model or computational intelligence method. This combination permits an increase in the accuracy of the integrating technique, through the modeling of higher-order terms and other external forces not considered in the integrating technique. In this paper, neural networks have been used as time series forecasters in order to help two economic general perturbation theories describe the motion of an orbiter only perturbed by the Earth’s oblateness.


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