Viento Solar
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Solar Storms
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Author : Tobi Stanton-Stewart
language : en
Publisher: The Rosen Publishing Group, Inc
Release Date : 2002-01-01
Solar Storms written by Tobi Stanton-Stewart and has been published by The Rosen Publishing Group, Inc this book supported file pdf, txt, epub, kindle and other format this book has been release on 2002-01-01 with Science categories.
Examines the characteristics and importance of the sun and how sunspots, solar wind, and solar storms affect the earth.
Solar Wind
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Author : Carlos Daniel Escaropa Borrega
language : en
Publisher:
Release Date : 2012
Solar Wind written by Carlos Daniel Escaropa Borrega and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012 with Solar wind categories.
In this book, the authors present current research in the study of the emission, technologies and impact of solar wind. The topics include the possible impact of the astronomical aspects of the violent cyclonic motions in the Earth's atmosphere; planetary beat, solar wind and terrestrial climate; and much more.
Viento Solar
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Author : José Rafael Echeverría Zeledón
language : es
Publisher:
Release Date : 2012
Viento Solar written by José Rafael Echeverría Zeledón and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012 with categories.
The Sun The Solar Wind And The Heliosphere
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Author : Mari Paz Miralles
language : en
Publisher: Springer Science & Business Media
Release Date : 2011-01-06
The Sun The Solar Wind And The Heliosphere written by Mari Paz Miralles 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 2011-01-06 with Science categories.
This volume represents the state of the art of the science covered by the International Association of Geomagnetism and Aeronomy (IAGA) Division IV: Solar Wind and Interplanetary Field. It contains a collection of contributions by top experts addressing and reviewing a variety of topics included under the umbrella of the division. It covers subjects that extend from the interior of the Sun to the heliopause, and from the study of physical processes in the Sun and the solar wind plasma to space weather forecasts. The book is organized in 6 parts: the solar interior, the solar atmosphere, the heliosphere, heliophysical processes, radio emissions, and coordinated science in the Sun-Earth system. In addition, we highlight some of the results presented during the IAGA Division IV symposia in the 11th Scientific Assembly of IAGA in Sopron, Hungary, on 23-30 August 2009, which was planned simultaneously with this book.
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.
Viento Solar
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Author : Rubén Derlis
language : es
Publisher:
Release Date : 1997
Viento Solar written by Rubén Derlis and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1997 with categories.
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.
Solar Plasma Wind Earth Currents And Diurnal Magnetic Field Variations
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Author : Hermann Poeverlein
language : en
Publisher:
Release Date : 1965
Solar Plasma Wind Earth Currents And Diurnal Magnetic Field Variations written by Hermann Poeverlein and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1965 with Earth currents categories.
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."
The Solar Wind And The Earth
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Author : Syun-Ichi Akasofu
language : en
Publisher: Springer
Release Date : 1989-11-30
The Solar Wind And The Earth written by Syun-Ichi Akasofu and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 1989-11-30 with Science categories.
As a star, the sun is continuously emitting an enormous amount of energy 33 into space, up to as much as 3. 9 X 10 erg/ s. This energy emission consists of three modes. Almost all the energy is emitted in the form of the familiar black-body radiation, commonly called sunlight. Although the amount of energy emitted is small, the sun also emits x rays, extreme ultraviolet (EUV), and UV radiations, which are absorbed above the earth's stratosphere. These constitute the second mode of solar energy, separate from the black-body radiation that penetrates the lower layers of the atmosphere. The sun has another important mode of energy emission in which the energy is carried out by charged particles. These particles have a very wide range of energies, from less than I keY to more than I GeV. Because of this wide range, it is convenient to group them into two components: particles with energies greater than 10 keY and the lower-energy particles. The former are generally referred to as solar protons or solar cosmic rays; their emission is associated with active features on the sun. Their interaction with the atmosphere is similar to that of the x ray and EUV radiation. Low-energy particles constitute plasma, a gas of equal numbers of positive and negative particles. Actually, this plasma is the outermost part of the solar atmosphere, namely the corona, which blows out continuously . For this reason, the plasma flow is called the solar wind.