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Solar Surface Magnetism

Solar Surface Magnetism

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"Solar Surface Magnetism" by Robert J. Rutten, Carolus J. Schrijver is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection and magnetic field in the photosphere regulates the field dispersal and drives the instabilities which heat the outer solar atmosphere. This book presents a synthesis between observers and theorists, both with regard to the magnetic elements which make up solar magnetic fields (ranging from tiny flux tubes to whole active regions), and to the surface patterns in which these elements display properties of the subsurface dynamo.

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Best For: Researchers and students in solar physics and astrophysics
Focus: The dynamics of solar surface magnetic flux and its role in solar interior processes and atmospheric heating
Covers: Magnetic elements on the solar surface, convection and magnetic field interactions in the photosphere, and the resulting instabilities affecting the solar atmosphere
Why It Matters: Understanding solar surface magnetism is key to explaining solar interior activity and the heating mechanisms of the outer solar atmosphere

"Solar Surface Magnetism" by Robert J. Rutten, Carolus J. Schrijver 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: Robert J. Rutten, Carolus J. Schrijver

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.

While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection and magnetic field in the photosphere regulates the field dispersal and drives the instabilities which heat the outer solar atmosphere. This book presents a synthesis between observers and theorists, both with regard to the magnetic elements which make up solar magnetic fields (ranging from tiny flux tubes to whole active regions), and to the surface patterns in which these elements display properties of the subsurface dynamo.

AuthorRobert J. Rutten, Carolus J. Schrijver
PublisherSpringer Science & Business Media
Published1994
ISBN-139780792328452
BindingHardcover
Pages560
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesNATO Asi Series. Series C, Mathematical and Physical Science

Format: Hardcover

Length: 560 pages

Language: English

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