The Acceleration Of Solar Wind Protons And Heavy Ions
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The Acceleration Of Solar Wind Protons And Heavy Ions
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Author :
language : en
Publisher:
Release Date : 2007
The Acceleration Of Solar Wind Protons And Heavy Ions written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2007 with categories.
Solar Wind Acceleration
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Author : Yuri V. Pisanko
language : en
Publisher: Cambridge Scholars Publishing
Release Date : 2022-03-14
Solar Wind Acceleration written by Yuri V. Pisanko and has been published by Cambridge Scholars Publishing this book supported file pdf, txt, epub, kindle and other format this book has been release on 2022-03-14 with Education categories.
In addition to sunshine, the Sun emits about one trillion tons of ionized hydrogen per second into the interplanetary space, a phenomenon known as solar wind. This book systematizes the knowledge of the solar wind acceleration region, which is, figuratively speaking, the space weather “kitchen” similar to the Mexican gulf (where the Gulf Stream originates). The processing of unique scientific information about the solar wind at heliocentric distances up to three solar radii obtained from receiving antennas directed almost to the Sun (a challenging technical task itself) during telecommunication sessions with “Mars-2”, “Mars-4”, “Venera-10”, “Venera-15”, and “Venera-16” spacecraft, along with original approaches for modelling the solar wind acceleration region, underlie the factual basis for the book.
The Acceleration Of Solar Wind Protons And Heavy Ions
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Author : A. O. Benz
language : en
Publisher:
Release Date : 1982
The Acceleration Of Solar Wind Protons And Heavy Ions written by A. O. Benz and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1982 with Solar wind categories.
Coronal Holes And Solar Wind Acceleration
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Author : John Kohl
language : en
Publisher: Springer Science & Business Media
Release Date : 1999-08-31
Coronal Holes And Solar Wind Acceleration written by John Kohl and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 1999-08-31 with Science categories.
The SOHO-7 Workshop was held from 28 September through 1 October 1998 at the Asticou Inn in Northeast Harbor, Maine. The primary topic of this Workshop was the impact of SOHO observations on our understanding of the nature and evolution of coronal holes and the acceleration and composition of the solar wind. The presentations and discussions occasionally went beyond this topic to include the impact of the reported research on other solar structures and the heliosphere. SOHO (the Solar and Heliospheric Observatory), a project of international cooperation between ESA and NASA, was launched in December 1995 and began its science operations during the first few months of 1996. To many solar and space physicists, it was a great advantage that SOHO began itscomprehensive look at the Sun during the 1996 solar minimum. The qualitatively simple two-phase corona, with polar coronal holes expanding into the high-speed solar wind, and a steady equatorial streamer belt related somehow to the stochastic slow-speed solar wind, allowed various SOHO diagnostics to be initiated with a reasonably well understoodcircumsolar geometry. The analysis of subsequentSOHO measurements made during the rising phase of solar cycle 23 will continue to benefit from what has been learned from the first two years of data.
Basics Of The Solar Wind
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Author : Nicole Meyer-Vernet
language : en
Publisher: Cambridge University Press
Release Date : 2007-01-18
Basics Of The Solar Wind written by Nicole Meyer-Vernet and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2007-01-18 with Science categories.
The Sun continually ejects matter into space, blowing a huge bubble of supersonic plasma. This solar wind bathes the whole solar system and shapes all planetary environments. The growth of space technology has considerably increased our knowledge of this medium. This 2007 book presents an introduction to the subject, starting with basic principles and including all the latest advances from space exploration and theory. It contains a short introduction to plasma physics and discusses the structure of the solar interior and atmosphere, the production of solar wind and its perturbations. It explains the objects of the Solar System, from dust to comets and planets, and their interaction with the solar wind. The final sections explore the astrophysical point of view. The topics are treated at various levels of difficulty both qualitatively and quantitatively. This book will appeal to graduate students and researchers in earth and atmospheric sciences, and astrophysics.
Exploring The Solar Wind
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Author : Marian Lazar
language : en
Publisher: BoD – Books on Demand
Release Date : 2012-03-21
Exploring The Solar Wind written by Marian Lazar and has been published by BoD – Books on Demand this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-03-21 with Science categories.
This book consists of a selection of original papers of the leading scientists in the fields of Space and Planetary Physics, Solar and Space Plasma Physics with important contributions to the theory, modeling and experimental techniques of the solar wind exploration. Its purpose is to provide the means for interested readers to become familiar with the current knowledge of the solar wind formation and elemental composition, the interplanetary dynamical evolution and acceleration of the charged plasma particles, and the guiding magnetic field that connects to the magnetospheric field lines and adjusts the effects of the solar wind on Earth. I am convinced that most of the research scientists actively working in these fields will find in this book many new and interesting ideas.
The Solar Wind
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Author : J. R. Herring
language : en
Publisher:
Release Date : 1960
The Solar Wind written by J. R. Herring and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1960 with Solar wind categories.
"Parker's model of a spherically expanding corona, the "solar wind," is compared with D.E. Blackwell's observations of the 1954 minimum equatorial corona. A significant discrepancy is found between the predicted and the observed electron densities at distances from the sun greater than 20 solar radii. Blackwell's data are found to be consistent with a model in which the corona expands mostly within a disk less than 25 solar radii thick, lying within the sun's equatorial plane. The thickness of the disk as a function of distance from the sun is qualitatively explained in terms of magnetic pressure. The solar wind is found to have a considerable effect on the lunar atmosphere. First, the calculated density of the lunar atmosphere is greatly reduced by collisions with protons in the solar wind. If the flux of particles in this wind has the conventional values ranging between 10(exp 10) to 10(exp 11) per sq cm-sec, the calculations yield a lunar pressure of 10(exp -13) atmosphere of argon, in agreement with the value predicted by Elsmore and Whitfield on the basis of observations on the occultation of radio stars. Second, following a suggestion by Gold, it was found that the collisions of solar-wind protons with the lunar surface produce an atmosphere of cold neutral hydrogen with a density of 10(exp 5) per cu cm at the lunar surface. The density falls off at greater distances in accordance with the inverse-square law. Estimates indicate that the interaction of solar particles with the neutral hydrogen will produce an extended lunar ionosphere with a density of the order of 400 protons/cu cm in the vicinity of the moon."
Solar Wind Three
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Author : Christopher T. Russell
language : en
Publisher:
Release Date : 1974
Solar Wind Three written by Christopher T. Russell and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1974 with Solar wind categories.
The Acceleration Of Solar Wind Protons And Heavy Ions
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Author : Arnold Otto Benz
language : en
Publisher:
Release Date : 1973
The Acceleration Of Solar Wind Protons And Heavy Ions written by Arnold Otto Benz and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1973 with Astrophysics categories.
Coronal Expansion And Solar Wind
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Author : A. J. Hundhausen
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06
Coronal Expansion And Solar Wind written by A. J. Hundhausen and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.
Little more than ten years have passed since spaceprobe-borne instruments con clusively demonstrated the existence of the solar wind. These observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interplanetary plasma near the orbit of the earth are now known in great detail. The theory of the coronal ex pansion has also been highly refilled both in the sense of including additional physical processes, and of treating more realistic (time-dependent and non spheri cally-symmetric) coronal boundary conditions. The present volume is an attempt to synthesize the solar wind observations and coronal expansion models from this decade of rapid development. The ultimate goal is, of course, the interpretation of observed solar wind phenomena as the effects of basic physical processes occurring in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "large-scale" features revealed by the observations. It requires extensive use of the concepts and methods of fluid mechanics.