Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-25T20:23:41.113Z Has data issue: false hasContentIssue false
  • English
  • Français

To kinetic modeling of solar wind over magnetoactive regions and beyond

Published online by Cambridge University Press:  14 March 2005

V. M. Gubchenko ,
V. V. Zaitsev ,
H. K. Biernat ,
M.L. Khodachenko  and
H. O. Rucker
V. M. Gubchenko
Affiliation:
Institute of Applied Physics, Russian Academy of Science, Nizhny Novgorod, email: [email protected]
V. V. Zaitsev
Affiliation:
Institute of Applied Physics, Russian Academy of Science, Nizhny Novgorod, email: [email protected]
H. K. Biernat
Affiliation:
Space Research Institute, Austrian Academy of Science, Graz, email: [email protected]
M.L. Khodachenko
Affiliation:
Space Research Institute, Austrian Academy of Science, Graz, email: [email protected]
H. O. Rucker
Affiliation:
Space Research Institute, Austrian Academy of Science, Graz, email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We model hot collisionless solar corona/slow solar wind (SW) by kinetic Vlasov equation. The equatorial region with an unprescribed magnetic field is under electromagnetic action, and we have formation of a 3D Quasi-Stationary Coronal Structures (QSCS) in the current-carrying (CC) plasma with SW flows. The QSCS are generated via electromagnetic mode development in plasma having anisotropic velocity distribution function (VDF). As a result we get streamers like stratification mode, CMEs like tearing mode and heliospheric sheet like pinch mode in anisotropic plasma. The scales in the QSCS are defined via angle dependent magnetic Debye scale. The scale itself depends on value and sign of plasma anisotropy parameter which is calculated for postulated plasma VDF.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 105 - 106
Copyright
© 2004 International Astronomical Union