Preface: Plasma transport across magnetospheric boundaries
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F16%3A10334227" target="_blank" >RIV/00216208:11320/16:10334227 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1016/j.asr.2016.05.009" target="_blank" >http://dx.doi.org/10.1016/j.asr.2016.05.009</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.asr.2016.05.009" target="_blank" >10.1016/j.asr.2016.05.009</a>
Alternative languages
Result language
angličtina
Original language name
Preface: Plasma transport across magnetospheric boundaries
Original language description
A plasma entering the magnetosphere crosses two principal boundaries - the bow shock and magnetopause. The crossing of the bow shock significantly modifies plasma parameters as well as the direction and magnitude of the frozen-in interplanetary magnetic field (IMF) creating a key region - the magnetosheath - for a transfer of solar wind mass and momentum to the magnetosphere. A highly turbulent magnetosheath plasma and magnetic field then interact with the magnetopause and can penetrate deeper into the magnetosphere.
Czech name
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Czech description
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Classification
Type
O - Miscellaneous
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů