Nature of prominences and their role in space weather proceedings of the 300th symposium of the International Astronomical Union, held in Paris, France, June 10 - 16, 2013
session I-1.1.Prominence fine structure, dynamics, and seismologysession I-1.2.Prominence plasmasession I-1.3.Magnetic field : measurements and modelssession I.-1.4.Filament environmentsession I-1.5.Solar cycle evolution of prominences and eruptionssession II-2.1.Prominence destabilization, CMEs, 3D...
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| Format: | UnknownFormat |
| Sprache: | eng |
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Cambridge u.a.
Cambridge Univ. Press
2013
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| Online Zugang: | Inhaltsverzeichnis |
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Tag hinzufügen | Zusammenfassung: | session I-1.1.Prominence fine structure, dynamics, and seismologysession I-1.2.Prominence plasmasession I-1.3.Magnetic field : measurements and modelssession I.-1.4.Filament environmentsession I-1.5.Solar cycle evolution of prominences and eruptionssession II-2.1.Prominence destabilization, CMEs, 3D reconstructionssession II-2.2.CMEs and magentic clouds in the heliosphere and their impacts on Earth's environmentsession III.Stellar ejecta and impact on exoplanetssession IV.Instrumentation, missions, and techniquesConclusionPosters sessions I-IV. Solar prominences and filaments are large gaseous features extending outward hundreds of thousands of kilometres from the Sun's surface, which play an active role in space weather. Magnetic clouds and interplanetary coronal mass ejections associated with erupting prominences can produce severe perturbations in the Earth's near-space environment. IAU Symposium 300 presents a review of the state-of-the-art theoretical and numerical modelling of prominences and filaments, and their role in the dynamics of Sun-Earth relations. Observations from the latest international space-borne missions (Hinode, STEREO and SDO) and ground-based observatories are presented. The Symposium benefits not just newcomers to solar physics research but it shares the current status of our sophisticated solar analysis with the stellar community, now that huge prominences and CMEs have been detected in solar-type stars, and others, which will affect any exoplanets they host.-- |
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| Beschreibung: | XXI, 533 S. Ill., graph. Darst. |
| ISBN: | 1107045193 1-107-04519-3 9781107045194 978-1-107-04519-4 |