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Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium

Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium

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"Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium" by Jeffrey L. Linsky, Salvatore Serio, International Astronomical Union is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

The Physics of Solar and Stellar Coronae provides the first comprehensive summary of the physical processes and phenomena occurring in solar and stellar coronae as observed at X-ray and other wavelengths. The book provides an early summary of the spectacular new solar X-ray observations being obtained with the Yohkoh satellite that are dramatically changing our understanding of the dynamics of the solar corona. With the perspective of two years' observations at X-ray and extreme ultraviolet wavelengths by the ROSAT satellite, many authors present new insights into the basic physical processes occurring in the coronae of stars across the Hertzsprung--Russell Diagram including both pre-main sequence and post-main sequence stars. Detailed models for the hot plasmas typically contained in magnetic loops in both stellar and solar coronae are presented to explain X-ray data obtained with the earlier X-ray instruments on Skylab, SMM, Einstein, and EXOSAT. The book includes papers on coronal observations obtained at other wavelengths and papers of the history of Palermo Astronomical Observatory. The Physics of Solar and Stellar Coronae is intended for researchers in the fields of solar physics and stellar astrophysics and will be a useful resource book for graduate level astrophysics courses. (ABSTRACT) This is the first comprehensive summary of the physical processes and phenomena occurring in solar and stellar coronae. Spectacular new solar X-ray observations by the Yohkoh satellite and stellar observations by ROSAT are highlighted, together with theoretical papers and detailed analyses of earlier data from Skylab, SMM, Einstein, and EXOSAT. Included are papers on coronal observations at other wavelengths and on the history of Palermo Astronomical Observatory.

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Best For: Researchers and students in astrophysics and space science focusing on solar and stellar phenomena.
Focus: Physical processes and phenomena in solar and stellar coronae observed at X-ray and other wavelengths.
Covers: Solar X-ray observations from the Yohkoh satellite and their impact on understanding solar corona dynamics.
Why It Matters: Offers a comprehensive summary of new observational data that advances knowledge of solar and stellar coronae physics.

"Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium" by Jeffrey L. Linsky, Salvatore Serio, International Astronomical Union is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Jeffrey L. Linsky, Salvatore Serio, International Astronomical Union

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

The Physics of Solar and Stellar Coronae provides the first comprehensive summary of the physical processes and phenomena occurring in solar and stellar coronae as observed at X-ray and other wavelengths. The book provides an early summary of the spectacular new solar X-ray observations being obtained with the Yohkoh satellite that are dramatically changing our understanding of the dynamics of the solar corona. With the perspective of two years' observations at X-ray and extreme ultraviolet wavelengths by the ROSAT satellite, many authors present new insights into the basic physical processes occurring in the coronae of stars across the Hertzsprung--Russell Diagram including both pre-main sequence and post-main sequence stars. Detailed models for the hot plasmas typically contained in magnetic loops in both stellar and solar coronae are presented to explain X-ray data obtained with the earlier X-ray instruments on Skylab, SMM, Einstein, and EXOSAT. The book includes papers on coronal observations obtained at other wavelengths and papers of the history of Palermo Astronomical Observatory. The Physics of Solar and Stellar Coronae is intended for researchers in the fields of solar physics and stellar astrophysics and will be a useful resource book for graduate level astrophysics courses. (ABSTRACT) This is the first comprehensive summary of the physical processes and phenomena occurring in solar and stellar coronae. Spectacular new solar X-ray observations by the Yohkoh satellite and stellar observations by ROSAT are highlighted, together with theoretical papers and detailed analyses of earlier data from Skylab, SMM, Einstein, and EXOSAT. Included are papers on coronal observations at other wavelengths and on the history of Palermo Astronomical Observatory.

AuthorJeffrey L. Linsky, Salvatore Serio, International Astronomical Union
PublisherSpringer Science & Business Media
Published1993
ISBN-139780792323464
BindingHardcover
Pages688
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesSynthese Library (Hardcover)

Format: Hardcover

Length: 688 pages

Language: English

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