Dynamic Changes of Magnetopause Locations Under Different Upstream Conditions

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F10%3A10080632" target="_blank" >RIV/00216208:11320/10:10080632 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Dynamic Changes of Magnetopause Locations Under Different Upstream Conditions

Original language description

Present magnetopause models describe the magnetopause location as a function of the solar wind dynamic pressure and IMF BZ component. However, the crossings observed by spacecraft are often far away from the predicted locations and it suggests that otherIMF components and/or other factors can be important under particular circumstances. We have found that magnetopause location strongly dependence on the IMF cone angle.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BL - Plasma physics and discharge through gases

OECD FORD branch

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Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach

Publication year

2010

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

WDS'10 Proceedings of Contributed Papers: Part II - Physics of Plasmas and Ionized Media

ISBN

978-80-7378-140-8

ISSN

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e-ISSN

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Number of pages

6

Pages from-to

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Publisher name

Matfyzpress

Place of publication

Praha

Event location

Praha

Event date

Jun 1, 2010

Type of event by nationality

EUR - Evropská akce

UT code for WoS article

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