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RAS PhysicsАстрономический журнал Astronomy Reports

  • ISSN (Print) 0004-6299
  • ISSN (Online) 3034-5170

3D NUMERICAL MODEL FOR STUDYING ELECTRON PRECIPITATION IN THE UPPER ATMOSPHERES OF VENUS-LIKE EXOPLANETS

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PII
S30345170S0004629925010034-1
DOI
10.7868/S3034517025010034
Publication type
Article
Status
Published
Authors
Andrey Zhilkin
  • Affiliation: Institute of Astronomy of the Russian Academy of Sciences
V. I Shematovich
  • Affiliation: Institute of Astronomy of the Russian Academy of Sciences
G. N Tsurikov
  • Affiliation: Institute of Astronomy of the Russian Academy of Sciences
D. V Bisikalo
  • Affiliation:
    Institute of Astronomy of the Russian Academy of Sciences
    National center of physics and mathematics
Volume/ Edition
Volume 102 / Issue number 1
Pages
35-48
Abstract
The paper presents a three-dimensional numerical model of solar wind plasma flow around a terrestrial planet that does not have its own magnetic field. The model is based on the approximation of multicomponent magnetohydrodynamics and takes into account ionization and recombination processes. The numerical model is validated using the example of the magnetosphere of Venus. Our model, in particular, allows us to calculate the structure and parameters of electron precipitation into the planet’s ionosphere. The developed model is supposed to be used to study observational manifestations of the potential biomarker NO in the atmospheres of exoplanets without their own magnetic field.
Keywords
Венера численное моделирование МГД ионосфера магнитосфера взаимодействие с солнечным ветром
Date of publication
22.01.2026
Year of publication
2026
Number of purchasers
0
Views
56

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