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Regularization of Equations of Motion of Celestial Bodies. 2. Correction of the KS-Coordinate System in Numerical Integration

✍ Scribed by S.M. Poleshchikov; A.A. Kholopov

Book ID
110221425
Publisher
SP MAIK Nauka/Interperiodica
Year
2000
Tongue
English
Weight
62 KB
Volume
34
Category
Article
ISSN
0038-0946

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## Abstract It is usual to use finite‐difference methods in carrying out the time integration of the equations of motion as adapted to the prediction of the large‐scale atmospheric pattern, and this implies a choice of the mesh length and time increment to be used. The effect of changing the size a