Peculiarities of magnetic barrier formation for southward and northward directions of the IMF-Reference-Cited by-同舟云学术

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Peculiarities of magnetic barrier formation for southward and northward directions of the IMF

Published:2015-11 Issue:11 Volume:120 Page:9471-9483
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Slivka K. Yu.¹,Semenov V. S.¹,Erkaev N. V.²³,Dmitrieva N. P.¹,Kubyshkin I. V.¹,Lammer H.⁴

Affiliation:

1. Earth Physics Department Saint Petersburg State University Saint Petersburg Russia

2. Institute of Computational Modelling SB RAS Krasnoyarsk Russia

3. Department of Applied Mechanics, Polytechnic Institute Siberian Federal University Krasnoyarsk Russia

4. Space Research Institute Austrian Academy of Sciences Graz Austria

Funder

RF President

Russian Foundation of Basic Research

Austrian Research Foundation FWF NFN

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021250

Reference23 articles.

1. Aspects of MHD flow about Venus

2. Geospace Environment Modeling (GEM) magnetic reconnection challenge: Resistive tearing, anisotropic pressure and Hall effects

3. Fully kinetic simulations of undriven magnetic reconnection with open boundary conditions

4. Reconnection onset in the magnetotail: Particle simulations with open boundary conditions

5. The Hall fields and fast magnetic reconnection

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