Solar MHD Theory and Observations

Solar MHD Theory and Observations PDF Author: National Solar Observatory/Sacramento Peak. Summer Workshop
Publisher:
ISBN:
Category : Science
Languages : en
Pages : 410

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Book Description


MHD Structures, Waves and Turbulence in the Solar Wind

MHD Structures, Waves and Turbulence in the Solar Wind PDF Author: C.-Y. Tu
Publisher: Springer
ISBN: 9789048145201
Category : Science
Languages : en
Pages : 0

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Book Description
This is the first book to give a comprehensive overview of recent observational and theoretical results on solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence, preference being given to phenomena in the inner heliosphere. Emphasis is placed on the progress made in the past decade in the understanding of the nature and origin of especially small-scale, compressible and incompressible fluctuations. Turbulence models describing the spatial transport and spectral transfer of the fluctuations in the inner heliosphere are discussed. Intermittency of solar wind fluctuations and their statistical distributions are investigated. Studies of the heating and acceleration effects of the turbulence on the background wind are critically surveyed. Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and perspectives for future research are outlined. The book is for graduate students and researchers in the field. Other target groups are scientists and professionals interested in space plasma physics and/or MHD turbulence.

MHD Structures, Waves and Turbulence in the Solar Wind

MHD Structures, Waves and Turbulence in the Solar Wind PDF Author: C.-Y. Tu
Publisher: Springer Science & Business Media
ISBN: 9401585415
Category : Science
Languages : en
Pages : 214

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Book Description
This is the first book to give a comprehensive overview of recent observational and theoretical results on solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence, preference being given to phenomena in the inner heliosphere. Emphasis is placed on the progress made in the past decade in the understanding of the nature and origin of especially small-scale, compressible and incompressible fluctuations. Turbulence models describing the spatial transport and spectral transfer of the fluctuations in the inner heliosphere are discussed. Intermittency of solar wind fluctuations and their statistical distributions are investigated. Studies of the heating and acceleration effects of the turbulence on the background wind are critically surveyed. Finally, open questions concerning the origin, nature and evolution of the fluctuations are listed, and perspectives for future research are outlined. The book is for graduate students and researchers in the field. Other target groups are scientists and professionals interested in space plasma physics and/or MHD turbulence.

Solar MHD Theory and Observations

Solar MHD Theory and Observations PDF Author: National Solar Observatory/Sacramento Peak Summer Workshop
Publisher:
ISBN: 9781583812884
Category :
Languages : en
Pages : 366

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Solar Magnetohydrodynamics

Solar Magnetohydrodynamics PDF Author: E.R. Priest
Publisher: Springer
ISBN: 9027718334
Category : Science
Languages : en
Pages : 469

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Book Description
I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im mediate start 'while your ideas are still fresh'. The book grew out of a postgraduate lecture course at St Andrews, and the resulting period of gestation or 'being with monograph' has lasted several years. The Sun is an amazing object, which has continued to reveal completely unexpected features when observed in greater detail or at new wavelengths. What riches would be in store for us if we could view other stars with as much precision! Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. In the 'old days' the solar atmosphere was regarded as a static, plane-parallel structure, heated by the dissipation of sound waves and with its upper layer expanding in a spherically symmetric manner as the solar wind. Outside of sunspots the magnetic field was thOUght to be unimportant with a weak uniform value of a few gauss.

Magnetohydrodynamics of the Sun

Magnetohydrodynamics of the Sun PDF Author: Eric Priest
Publisher: Cambridge University Press
ISBN: 0521854717
Category : Science
Languages : en
Pages : 581

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Book Description
This advanced textbook reviews the complex interaction between the Sun's plasma atmosphere and its magnetic field.

Reconnection of Magnetic Fields

Reconnection of Magnetic Fields PDF Author: J. Birn
Publisher: Cambridge University Press
ISBN: 1139460102
Category : Science
Languages : en
Pages : 302

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Book Description
The reconnection of magnetic fields is one of the most fascinating processes in plasma physics, responsible for phenomena such as solar flares and magnetospheric substorms. The concept of reconnection has developed through recent advances in exploring the magnetospheres of the Sun and Earth through theory, computer simulations and spacecraft observations. The great challenge in understanding it stems from balancing the large volumes of plasma and magnetic fields involved with the energy release with the physical mechanism which relies on the strongly localized behavior of charged particles. This book, edited by and with contributions from leading scientists in the field, provides a comprehensive overview of recent theoretical and observational findings concerning the physics of reconnection and the complex structures that may give rise to, or develop from, reconnection. It is intended for researchers and graduate students interested in the dynamics of plasmas.

Magnetohydrodynamics of the Sun

Magnetohydrodynamics of the Sun PDF Author: Eric Priest
Publisher: Cambridge University Press
ISBN: 110778266X
Category : Science
Languages : en
Pages : 581

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Book Description
Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at www.cambridge.org/9780521854719.

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere PDF Author: Xueshang Feng
Publisher: Springer
ISBN: 9811390819
Category : Science
Languages : en
Pages : 772

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Book Description
The book covers intimately all the topics necessary for the development of a robust magnetohydrodynamic (MHD) code within the framework of the cell-centered finite volume method (FVM) and its applications in space weather study. First, it presents a brief review of existing MHD models in studying solar corona and the heliosphere. Then it introduces the cell-centered FVM in three-dimensional computational domain. Finally, the book presents some applications of FVM to the MHD codes on spherical coordinates in various research fields of space weather, focusing on the development of the 3D Solar-InterPlanetary space-time Conservation Element and Solution Element (SIP-CESE) MHD model and its applications to space weather studies in various aspects. The book is written for senior undergraduates, graduate students, lecturers, engineers and researchers in solar-terrestrial physics, space weather theory, modeling, and prediction, computational fluid dynamics, and MHD simulations. It helps readers to fully understand and implement a robust and versatile MHD code based on the cell-centered FVM.

The Internal Solar Angular Velocity

The Internal Solar Angular Velocity PDF Author: National Solar Observatory (U.S.). Summer Symposium
Publisher: Springer
ISBN:
Category : Gardening
Languages : en
Pages : 396

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Book Description
Proceedings of the 8th NSO Summer Symposium held at Sacramento Peak, New Mexico, August 11-14, 1986