Cold Ions Observed near Magnetopause and their Effects on Reconnection | The Solar Wind-Magnetosphere-Ionosphere Coupling

Sun Hee Lee (u. a.)

ISBN 10: 3659834572 ISBN 13: 9783659834578
Edité par LAP LAMBERT Academic Publishing, 2016
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Cold Ions Observed near Magnetopause and their Effects on Reconnection | The Solar Wind-Magnetosphere-Ionosphere Coupling | Sun Hee Lee (u. a.) | Taschenbuch | 164 S. | Englisch | 2016 | LAP LAMBERT Academic Publishing | EAN 9783659834578 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu. N° de réf. du vendeur 103936065

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Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined.

Présentation de l'éditeur: Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined.

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Titre : Cold Ions Observed near Magnetopause and ...
Éditeur : LAP LAMBERT Academic Publishing
Date d'édition : 2016
Reliure : Taschenbuch
Etat : Neu

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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Lee Sun HeeSun Hee Lee received her PhD in space physics from the University of Alaska Fairbanks. She worked with Professor Hui Zhang at the Geophysical Institute and Physics Department of UAF from 2010 to 2015. She was awarded NASA . N° de réf. du vendeur 158605955

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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 164 pp. Englisch. N° de réf. du vendeur 9783659834578

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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined. 164 pp. Englisch. N° de réf. du vendeur 9783659834578

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Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined. N° de réf. du vendeur 9783659834578

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