Mathematical model of Martian wind disturbances

Аuthors

Dunchenko O. M.

Abstract

Researches of the Martian atmosphere by automatic interplanetary stations revealed a sufficiently strong wind effects in the lower 20-25 km layer of the planet atmosphere. In this paper is carried out the analysis the probabilistic characteristics the field of wind speed based on the statistical experimental data. The mathematical model of wind disturbances is considered in the form of canonical decomposition.

Keywords:

spacecraft; Mars; wind disturbances; confidence intervals; canonical decomposition

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