Energy Storage and Release through the Solar Activity Cycle
Models Meet Radio Observations
(Sprache: Englisch)
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...
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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.
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.
Klappentext zu „Energy Storage and Release through the Solar Activity Cycle “
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.
Inhaltsverzeichnis zu „Energy Storage and Release through the Solar Activity Cycle “
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.
Autoren-Porträt
Dr. Marqué completed his PhD at the Paris Observatory in France, focusing on the imagery of the quiet solar corona. His research is also oriented towards radio signatures of solar eruptive events. He is currently working at the Royal Observatory of Belgium in Brussels, where he is in charge of ground based solar radio observations.Dr. Nindos is an assistant professor at the Physics Department of the University of Ioannina, Greece. His research interests are generally focused on solar physics, with particular interest to solar radio astronomy and solar magnetic fields.
Dr. van Driel-Gesztelyi has been one of three Editor in Chiefs of Solar Physics since 2005. She has a broad (principally observational) expertise in solar physics, including solar magnetic fields, active region evolution and activity phenomena (flares, eruptions, coronal mass ejections, coronal heating). She obtained her PhD at Charles University in Prague and her DSci degree at the Hungarian Academy of Sciences (2004). She is currently (part-time) Reader at University College London, UK, associated astronomer at Paris Observatory, France and scientific consultant at Konkoly Observatory, Hungary.
Dr. Mandrini obtained her PhD at the University of Buenos Aires. At present, she is a Professor at the Department of Physics, Faculty of Exact and Natural Sciences, University of Buenos Aires and Principal Researcher at the National Council of Scientific and Technological Research in Argentina. She has been the Associate Editor of Solar Physics since 2008. She has a broad expertise in solar physics, mainly in solar magnetic fields, including magnetic field modeling, active region evolution and solar active phenomena (flares, coronal mass ejections).
Bibliographische Angaben
- 2012, VI, 230 Seiten, Masse: 16 x 24,1 cm, Gebunden, Englisch
- Herausgegeben: Christophe Marque, Alexander Nindos
- Verlag: Springer, Berlin
- ISBN-10: 1461444020
- ISBN-13: 9781461444022
- Erscheinungsdatum: 17.06.2012
Sprache:
Englisch
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