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Mhd Structures, Waves and Turbulence in the Solar Wind: Observations and Theories (Reprinted from Space Science Reviews, 73:1-2, 1995)

MHD Structures, Waves and Turbulence in the Solar Wind

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"MHD Structures, Waves and Turbulence in the Solar Wind" by C.-Y. Tu, Eckart Marsch is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and possible avenues and perspectives for future research are outlined.

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Best For: Researchers and students in astrophysics and space science focusing on solar wind phenomena.
Focus: Magnetohydrodynamic (MHD) structures, waves, and turbulence in the solar wind.
Covers: Origin, nature, and evolution of fluctuations in the solar wind, along with future research directions.
Why It Matters: Understanding these fluctuations is crucial for advancing knowledge of solar wind behavior and its impact on space weather.

"MHD Structures, Waves and Turbulence in the Solar Wind" by C.-Y. Tu, Eckart Marsch 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: C.-Y. Tu, Eckart Marsch

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.

Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and possible avenues and perspectives for future research are outlined.

AuthorC.-Y. Tu, Eckart Marsch
PublisherSpringer
Published1995-04-30
ISBN-139780792333456
BindingHardcover
Pages222
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System

Format: Hardcover

Length: 222 pages

Language: English

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