Energy Conversion and Particle Acceleration in the Solar Corona

Energy Conversion and Particle Acceleration in the Solar Corona PDF

Author: Karl-Ludwig Klein

Publisher: Springer

Published: 2008-01-11

Total Pages: 319

ISBN-13: 3540362428

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The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the sun, the present volume reviews the current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as non-specialist researchers from related areas and postgraduate students.

Energy Conversion and Particle Acceleration in the Solar Corona

Energy Conversion and Particle Acceleration in the Solar Corona PDF

Author: Karl-Ludwig Klein

Publisher: Springer

Published: 2003-02-27

Total Pages: 319

ISBN-13: 9783540002758

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The conversion of energy generated in the Sun's interior creates its hot corona and a wealth of dynamical phenomena such as flares and mass ejections. Based on recent significant progress in understanding magnetic reconnection and a wealth of new observations of energetic particle signatures from the Sun, the present volume reviews the current theoretical and experimental status in the field. Paying attention to both the details and the broader picture, this book addresses both the experienced researcher as well as nonspecialist researchers from related areas and postgraduate students in astrophsics.

The High Energy Solar Corona: Waves, Eruptions, Particles

The High Energy Solar Corona: Waves, Eruptions, Particles PDF

Author: Karl L. Klein

Publisher: Springer

Published: 2007-09-26

Total Pages: 284

ISBN-13: 3540715703

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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.

Plasma Physics of the Local Cosmos

Plasma Physics of the Local Cosmos PDF

Author: National Research Council

Publisher: National Academies Press

Published: 2004-06-06

Total Pages: 100

ISBN-13: 9780309092159

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Solar and space physics is the study of solar system phenomena that occur in the plasma state. Examples include sunspots, the solar wind, planetary magnetospheres, radiation belts, and the aurora. While each is a distinct phenomenon, there are commonalities among them. To help define and systematize these universal aspects of the field of space physics, the National Research Council was asked by NASA's Office of Space Science to provide a scientific assessment and strategy for the study of magnetized plasmas in the solar system. This report presents that assessment. It covers a number of important research goals for solar and space physics. The report is complementary to the NRC report, The Sun to the Earthâ€"and Beyond: A Decadal Research Strategy for Solar and Space Physics, which presents priorities and strategies for future program activities.

The Sun from Space

The Sun from Space PDF

Author: Kenneth R. Lang

Publisher: Springer Science & Business Media

Published: 2008-10-20

Total Pages: 583

ISBN-13: 3540769536

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The First Edition of The Sun from Space, completed in 1999, focused on the early accomplishments of three solar spacecraft, SOHO, Ulysses, and Yohkoh, primarily during a minimum in the Sun’s 11-year cycle of magnetic activity. The comp- hensive Second Edition includes the main ndings of these three spacecraft over an entire activity cycle, including two minima and a maximum, and discusses the signi cant results of six more solar missions. Four of these, the Hinode, RHESSI, STEREO, and TRACE missions were launched after the First Edition was either nished or nearly so, and the other two, the ACE and Wind spacecraft, extend our investigations from the Sun to its varying input to the Earth. The Second Edition does not contain simple updates or cosmetic patch ups to the material in the First Edition. It instead contains the relevant discoveries of the past decade, integrated into chapters completely rewritten for the purpose. This provides a fresh perspective to the major topics of solar enquiry, written in an enjoyable, easily understood text accessible to all readers, from the interested layperson to the student or professional.

Magnetic Fields in the Solar Atmosphere

Magnetic Fields in the Solar Atmosphere PDF

Author: Jacques Maurice Beckers

Publisher:

Published: 1976

Total Pages: 40

ISBN-13:

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This paper describes the magnetic field configurations observed in the solar atmosphere including the corona and the solar wind. The techniques for observing solar magnetic fields are briefly reviewed. The significance of Alfven waves in transporting energy is stressed. (Author).

Solar Magnetic Phenomena

Solar Magnetic Phenomena PDF

Author: A. Hanslmeier

Publisher: Springer Science & Business Media

Published: 2006-03-30

Total Pages: 297

ISBN-13: 1402029624

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The concept of summerschools and workshops at the Kanzelh· ohe · Solar Observatory, Karn · · ten, Austria, devotedtoup-to-datetopicsinsolarphysics has been proven to be extremely successful, and thus in August/September 2003 the third combined summerschool and workshop was held there. This book contains the proceedings of the Summerschool and Wo- shop "Solar Magnetic Phenomena" held from 25 August to 5 September 2003 at the Solar Observatory Kanzelh· ohe, · which belongs to the Institute for Geophysics, Astrophysics and Meteorology of the University of Graz, Austria. The book contains the contributions from six invited lecturers. They give an overview on the following topics: observations of the pho- sphere and chromosphere, solar?are observations and theory, coronal mass ejections and the relevance of magnetic helicity, high-energy radiation from the Sun, the physics of solar prominences and highlights from the SOHO mission. The lectures contain about 25 to 30 pages each and provide a valuableintroduction to the topics mentioned above. The comprehensive lists ofreferences at theendof each contribution enablethe interested reader to go into more detail. The second part of the book contains contributed papers. These - pers were presented anddiscussed in theworkshop sessions during the afternoons. The sessions stimulated intensive discussions between the p- ticipants and lecturers

Physics of the Solar Corona

Physics of the Solar Corona PDF

Author: Markus Aschwanden

Publisher: Springer Science & Business Media

Published: 2006-08-26

Total Pages: 924

ISBN-13: 3540307664

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A thorough introduction to solar physics based on recent spacecraft observations. The author introduces the solar corona and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth.

Transport and Energy Conversion in the Heliosphere

Transport and Energy Conversion in the Heliosphere PDF

Author: J.-P. Rozelot

Publisher: Springer

Published: 2008-01-11

Total Pages: 218

ISBN-13: 3540451668

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The book contains courses taught to a public of Ph.D. students, post-docs and confirmed researchers in all fields of heliospheric plasma physics. It aims at identifying physical issues which are common to two different fields of astronomy: solar and magnetospheric physics. Emphasis is given to basic processes of transport and conversion of energy: magnetic reconnection is discussed in detail from the viewpoints of MHD and kinetic physics. Processes of charged particle acceleration are reviewed and compared with recent observations. The subject is introduced by a summary of MHD, and the basic structures and parameters of the solar atmosphere, terrestrial ionosphere and magnetosphere are reviewed. The book combines a pedagogic and comprehensive presentation of physical issues and raises fully open questions, with the complementary and sometimes conflicting views of geophysicists and solar physicists. The book's focus, while basic, opens new avenues.