Energy Storage and Release through the Solar Activity Cycle Models Meet Radio Observations /

For nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma parameters have been measured from the l...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor Corporativo: SpringerLink (Online service)
Otros Autores: Marque, Christophe (Editor ), Nindos, Alexander (Editor )
Formato: Electrónico eBook
Idioma:Inglés
Publicado: New York, NY : Springer New York : Imprint: Springer, 2012.
Edición:1st ed. 2012.
Temas:
Solar system.
Atmospheric science.
Space Physics.
Atmospheric Science.
Acceso en línea:Texto Completo

MARC

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245 1 0 |a Energy Storage and Release through the Solar Activity Cycle  |h [electronic resource] :  |b Models Meet Radio Observations /  |c edited by Christophe Marque, Alexander Nindos. 
250 |a 1st ed. 2012. 
264 1 |a New York, NY :  |b Springer New York :  |b Imprint: Springer,  |c 2012. 
300 |a VI, 230 p.  |b online resource. 
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505 0 |a From the Contents: Radio Emission of the Quiet Sun and Active Regions (Invited Review).-Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare -- Location of Decimetric Pulsations in Solar Flares -- Millisecond Radio Spikes in the Decimetric Band -- Magnetoacoustic Wave Trains in the 11 July 2005 Radio Event with Fiber Bursts -- Quasi-periodic Oscillations of Solar Active Regions in Connection with Their Flare Activity-NoRH Observations -- Electron Spikes, Type III Radio Bursts and EUV Jets on 22 February 2010 -- Relation Between the 3D-Geometry of the Coronal Wave and Associated CME During the 26 April 2008 Event. 
520 |a For nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma parameters have been measured from the low chromosphere to the upper corona and interplanetary medium. This book presents current research in solar radio astronomy and shows how well it fits in the exceptional scientific context brought by the current space solar observatories. It essentially contains contributed research and review papers presented during the 2010 Community of European Solar Radio Astronomers (CESRA) meeting, which took place in Belgium in June 2010. This book is aimed at graduate students and researchers working in solar physics and space science. Previously published in Solar Physics journal, Vol. 273/2, 2011. 
650 0 |a Solar system. 
650 0 |a Atmospheric science. 
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650 2 4 |a Atmospheric Science. 
700 1 |a Marque, Christophe.  |e editor.  |4 edt  |4 http://id.loc.gov/vocabulary/relators/edt 
700 1 |a Nindos, Alexander.  |e editor.  |4 edt  |4 http://id.loc.gov/vocabulary/relators/edt 
710 2 |a SpringerLink (Online service) 
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776 0 8 |i Printed edition:  |z 9781461444022 
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950 |a Physics and Astronomy (SpringerNature-11651) 
950 |a Physics and Astronomy (R0) (SpringerNature-43715) 

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