Magnetic Reconnection: Theoretical and Observational Perspectives
Autor William Lewis Editat de Spiro Antiochos, James Drakeen Limba Engleză Paperback – 22 feb 2014
This volume is aimed at researchers in solar physics, magnetospheric physics and plasma physics.
Previously published in Space Science Reviews journal, Vol. 160/1-4, 2011.
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Specificații
ISBN-13: 9781489986252
ISBN-10: 1489986251
Pagini: 176
Ilustrații: V, 168 p.
Dimensiuni: 155 x 235 x 9 mm
Greutate: 0.25 kg
Ediția:2012
Editura: Springer
Colecția Springer
Locul publicării:New York, NY, United States
ISBN-10: 1489986251
Pagini: 176
Ilustrații: V, 168 p.
Dimensiuni: 155 x 235 x 9 mm
Greutate: 0.25 kg
Ediția:2012
Editura: Springer
Colecția Springer
Locul publicării:New York, NY, United States
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Public țintă
ResearchCuprins
Preface.- The Diffusion Region in Collisionless Magnetic Reconnection.- Understanding the Dynamics of Magnetic Reconnection Layer.- Magnetic Reconnection in Extreme Astrophysical Environments.- Observed Aspects of Reconnection in Solar Eruptions.- Properties of Near-Earth Magnetic Reconnection from In-Situ Observations.- Reconnection and Waves: A Review with a Perspective.- Who Needs Turbulence? A Review of Turbulence Effects in the Heliosphere and on the Fundamental Process of Reconnection.
Notă biografică
William Lewis is the Principal Scientist at Southwest Research Institute. He has also been a member of Yosemite 2010 Program Committee.
Spiro Antiochos is an astrophysicist in the Heliophysics Division of NASA GSFC. His fields of expertise include theoretical solar physics and plasma physics. Primarily, his work consists of developing theoretical models to explain observations from NASA space missions. During his career he has worked on a number of problems related to the Sun and Heliosphere, in particular, the physics of magnetic-driven activity and the structure of the Sun's corona.
James Drake received his doctorate in Theoretical Physics in 1975. He remained at UCLA for a brief time as a post-doctoral scholar and then moved to the University of Maryland, first as a post-doctoral scholar and then as a member of the teaching faculty in the Department of Physics and the Institute for Physical Science and Technology. In recognition for his contributions to the field of plasma physics, he was granted fellowship status in the American Physical Society and was awarded a Humboldt Senior Scientist Research Award.
Spiro Antiochos is an astrophysicist in the Heliophysics Division of NASA GSFC. His fields of expertise include theoretical solar physics and plasma physics. Primarily, his work consists of developing theoretical models to explain observations from NASA space missions. During his career he has worked on a number of problems related to the Sun and Heliosphere, in particular, the physics of magnetic-driven activity and the structure of the Sun's corona.
James Drake received his doctorate in Theoretical Physics in 1975. He remained at UCLA for a brief time as a post-doctoral scholar and then moved to the University of Maryland, first as a post-doctoral scholar and then as a member of the teaching faculty in the Department of Physics and the Institute for Physical Science and Technology. In recognition for his contributions to the field of plasma physics, he was granted fellowship status in the American Physical Society and was awarded a Humboldt Senior Scientist Research Award.
Textul de pe ultima copertă
This volume covers different aspects of recent theoretical and observational work on magnetic reconnection, a fundamental plasma-physical process by which energy stored in a magnetic field is converted, often explosively, into heat and kinetic energy. This collection of papers from the fields of solar and space physics, astrophysics, and laboratory plasma physics is especially timely in view of NASA's upcoming Magnetospheric Multiscale mission, which will use Earth's magnetosphere as a laboratory to test, through in-situ measurement of the plasma, energetic particles, and electric and magnetic fields, the various and sometimes competing models and theories of magnetic reconnection.
This volume is aimed at researchers in solar physics, magnetospheric physics and plasma physics.
Previously published in Space Science Reviews journal, Vol. 160/1-4, 2011.
This volume is aimed at researchers in solar physics, magnetospheric physics and plasma physics.
Previously published in Space Science Reviews journal, Vol. 160/1-4, 2011.
Caracteristici
Examines the fundamental plasma-physical process of magnetic reconnection from an interdisciplinary perspective, reviewing recent reconnection research in the fields of solar and space physics, astrophysics, and laboratory plasma physics
Presents both theoretical and observational results relating to key questions in reconnection research
Discusses the phenomenon of reconnection in extreme astrophysical environments as well as in the more familiar magnetospheric, solar, and laboratory plasma environments
Presents both theoretical and observational results relating to key questions in reconnection research
Discusses the phenomenon of reconnection in extreme astrophysical environments as well as in the more familiar magnetospheric, solar, and laboratory plasma environments