Buch, Englisch, 284 Seiten, Format (B × H): 160 mm x 241 mm, Gewicht: 1310 g
Reihe: Lecture Notes in Physics
Buch, Englisch, 284 Seiten, Format (B × H): 160 mm x 241 mm, Gewicht: 1310 g
Reihe: Lecture Notes in Physics
ISBN: 978-3-540-71569-6
Verlag: Springer
An outgrow of an earlier workshop held by the community of European Solar Radio Astronomers (CESRA), this topical volume collects reviews on the current multiwavelength findings and perspectives from the space missions RHESSI, TRACE and SOTTO. The aspects of solar physics dealt with are particle acceleration during flares, large-scale disturbances, and coronal plasma physics.
Zielgruppe
Research
Autoren/Hrsg.
Fachgebiete
- Geowissenschaften Geologie Geophysik
- Naturwissenschaften Physik Angewandte Physik Astrophysik
- Geowissenschaften Geologie Geodäsie, Kartographie, Fernerkundung
- Naturwissenschaften Physik Quantenphysik Radioaktivität
- Naturwissenschaften Astronomie Kosmologie, Urknalltheorie
- Naturwissenschaften Physik Quantenphysik Teilchenphysik
- Naturwissenschaften Astronomie Astrophysik
- Naturwissenschaften Physik Quantenphysik Hochenergiephysik
- Geowissenschaften Geographie | Raumplanung Geodäsie, Kartographie, GIS, Fernerkundung
- Naturwissenschaften Physik Thermodynamik Plasmaphysik
- Naturwissenschaften Physik Angewandte Physik Geophysik
Weitere Infos & Material
Introduction: The High-energy Corona – Waves, Eruptions, Particles.- Introduction: The High-energy Corona – Waves, Eruptions, Particles.- Particle Acceleration During Flares.- Magnetic Complexity, Fragmentation, Particle Acceleration and Radio Emission from the Sun.- Review of Selected RHESSI Solar Results.- RHESSI Results – Time for a Rethink?.- Small Scale Energy Release and the Acceleration and Transport of Energetic Particles.- Large-scale Disturbances.- Large-scale Waves and Shocks in the Solar Corona.- Energetic Particles Related with Coronal and Interplanetary Shocks.- Particle Acceleration at the Earth’s Bow Shock.- On the Existence of Non-maxwellian Velocity Distribution Functions in the Corona and their Consequences for the Solar Wind Acceleration.- Recent Research: Large-scale Disturbances, their Origin and Consequences.- Plasma of the Solar Corona.- Quasi-periodic Pulsations as a Diagnostic Tool for Coronal Plasma Parameters.- Pulsating Solar Radio Emission.
