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Author : Donald J. Williams
Publisher : Unknown
Page : 0 pages
File Size : 47,8 Mb
Release : 1976
Category : Electronic
ISBN : 1118659023
Author : Anonim
Publisher : American Geophysical Union
Page : 523 pages
File Size : 48,5 Mb
Release : 2024-07-01
Category : Electronic
ISBN : 8210379456XXX
Author : Donald J. Williams
Publisher : Unknown
Page : 510 pages
File Size : 43,8 Mb
Release : 1976
Category : Mass transfer
ISBN : 1118658779
Author : Donald J. Williams
Publisher : Unknown
Page : 640 pages
File Size : 41,8 Mb
Release : 1976
Category : Cosmic magnetic fields
ISBN : UCAL:B3764556
Author : Tadanori Ondoh,Katsuhide Marubashi
Publisher : IOS Press
Page : 322 pages
File Size : 40,8 Mb
Release : 2001
Category : Atmosphere, Upper
ISBN : 4274903842
Author : Nicole Meyer-Vernet
Publisher : Cambridge University Press
Page : 451 pages
File Size : 43,7 Mb
Release : 2007-01-18
Category : Science
ISBN : 9781139461559
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.
Author : Rainer Schwenn,Eckart Marsch
Publisher : Springer Science & Business Media
Page : 360 pages
File Size : 49,8 Mb
Release : 2013-06-29
Category : Science
ISBN : 9783642753640
Physics of the Inner Heliosphere gives for the first time a comprehensive and complete summary of our knowledge of the inner solar system. Using data collected over more than 11 years by the HELIOS twin solar probes, one of the most successful ventures in unmanned space exploration, the authors have compiled six extensive reviews of the physical processes of the inner heliosphere and their relation to the solar atmosphere. Researchers and advanced students in space and plasma physics, astronomy, and solar physics will be surprised to see just how closely the heliosphere is tied to, and how sensitively it depends on, the sun. Volume 2 deals with particles, waves, and turbulence, with chapters on: - magnetic clouds - interplanetary clouds - the solar wind plasma and MHD turbulence - waves and instabilities - energetic particles in the inner solar system
Author : J.G. Roederer
Publisher : Springer Science & Business Media
Page : 415 pages
File Size : 55,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400970960
Solar-Terrestrial Physics: The Study of Mankind's Newest Frontier Solar-Terrestrial Physics (STP) has been around for 100 years. However, it only became known as a scientific discipline under that name when the physical domain studied by STP became accessible to in situ observation and measurement by man or man-made instruments. Indeed, it was STP that provided the initial scientific driving force for the launching of man-made devices into extra-terrestrial space during the International Geophysical Year - aided of course by the genetically engrained drive of humans to expand their frontiers of knowledge, influence and dominance. We may define STP as the discipline dealing with the variable components of solar corpuscular and electromagnetic emissions, the physical processes governing their sources and their propagation through interplanetary space, and the physical-chemical processes related to their interaction with the Earth and other bodies in interplanetary space. Much of STP deals with fully-or partially-ionized gas flows and related energy, momentum and mass transfer in what now appears as one single system made up of distinct but strongly interacting parts, reaching from the photosphere out to the confines of the heliopause, engulfing planets and other solar system bodies, and dipping deep into 6 the Earth's atmosphere.
Author : Daniel Winterhalter,Mario Acuña,Alexander Zakharov
Publisher : Springer Science & Business Media
Page : 269 pages
File Size : 54,6 Mb
Release : 2013-06-05
Category : Science
ISBN : 9780306486043
Given that the question of an internal magnetic field is of fundamental importance to the understanding of Mars' formation and thermal evolution, and of the evolution of Mars' atmosphere, surprisingly few of the many spacecraft sent to Mars were equipped with instrumentation for such investigations. Of the 9 or so orbiters that have successfully archived Mars orbit, even if for a short period of time, only two have returned useful data about the magnetic field and about the plasma environment near Mars: The Phobos 2 spacecraft, and more recently, Mars Global Surveyor (MGS). With the discovery by MGS that Mars has large remnant magnetic field structures indicating an internal dynamo long extinct, the true nature of the past and present interaction between Mars and the solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions.
Author : Carolus J. Schrijver,Frances Bagenal,Jan J. Sojka
Publisher : Cambridge University Press
Page : 128 pages
File Size : 43,5 Mb
Release : 2016-03-17
Category : Science
ISBN : 9781316489789
Heliophysics is a fast-developing scientific discipline that integrates studies of the Sun's variability, the surrounding heliosphere, and the environment and climate of planets. This volume, the fourth in the Heliophysics collection, explores what makes the conditions on Earth 'just right' to sustain life, by comparing Earth to other solar system planets, by comparing solar magnetic activity to that of other stars, and by looking at the properties of evolving exoplanet systems. By taking an interdisciplinary approach and using comparative heliophysics, the authors illustrate how we can learn about our local cosmos by looking beyond it, and in doing so, also enable the converse. Supplementary online resources are provided, including lecture presentations, problem sets and exercise labs, making this ideal as a textbook for advanced undergraduate- and graduate-level courses, as well as a foundational reference for researchers in the many subdisciplines of helio- and astrophysics.
Author : Willard Paul Olson
Publisher : American Geophysical Union
Page : 665 pages
File Size : 49,6 Mb
Release : 1979
Category : Magnetosphere
ISBN : 9780875900216
Author : K.A. Naugol'nikh,L.A. Ostrovsky
Publisher : Springer Science & Business Media
Page : 528 pages
File Size : 48,8 Mb
Release : 1997-05-08
Category : Science
ISBN : 1563963388
Market: Acousticians, research scientists, instructors, and graduate and advanced undergraduate students in nonlinear acoustics. This book contains a collection of papers by authors of the Former Soviet Union. The topics covered are media with "structural" nonlinearities, optical generation of sound, acoustic beat-wave interactions, acoustic shock waves, thermal self-focusing of acoustic waves, solitons, statistical nonlinear acoustics, media with relaxation and oscillatory degrees of freedom, parametric arrays, and fluid cavitation.
Author : Andreas Keiling,Caitríona Jackman,Peter Delamere
Publisher : John Wiley & Sons
Page : 417 pages
File Size : 51,9 Mb
Release : 2015-02-02
Category : Science
ISBN : 9781118842348
All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. It is not only the strongly magnetized planets that have magnetotails. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosphere of its parent planet. The largest magnetotail of all in our solar system is the heliotail, the “magnetotail” of the heliosphere. The variety of solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions provide an outstanding opportunity to extend our understanding of the influence of these factors on magnetotail processes and structures. Volume highlights include: Discussion on why a magnetotail is a fundamental problem of magnetospheric physics Unique collection of tutorials on a large range of magnetotails in our solar system In-depth reviews comparing magnetotail processes at Earth with other magnetotail structures found throughout the heliosphere Collectively, Magnetotails in the Solar System brings together for the first time in one book a collection of tutorials and current developments addressing different types of magnetotails. As a result, this book should appeal to a broad community of space scientists, and it should also be of interest to astronomers who are looking at tail-like structures beyond our solar system.
Author : E. N. Parker
Publisher : Oxford University Press
Page : 860 pages
File Size : 43,9 Mb
Release : 2019-10-10
Category : Science
ISBN : 9780192565570
This well known and widely used landmark text explores the universal spontaneous generation of magnetic fields in astronomical bodies and the agitation of the bodies by those fields. The general properties of magnetic fields, their appearance throughout the astronomical universe, and the havoc they wreak are described in simple physical terms so as to define the broad scientific problem presented by magnetic fields. Then, with the physical problems clearly in mind, the theoretical effects are demonstrated with formal mathematical illustrations from the basic electromagnetic equations. Oxford Classic Texts in the Physical Sciences From James Clerk Maxwell's towering achievement Treatise on electricity and magnetism, to today's ground-breaking research, Oxford University Press has often been regarded as the publisher of first choice for generations of scientists. The legacy of this long publishing tradition is an unrivalled catalogue of past publications, some of which have been unavailable from us for many years. By popular demand, Oxford University Press is now reissuing some of its most celebrated science classics in the Oxford Classic Texts series. The titles to be included have been selected not only for their historic significance, but also for their enduring eloquence and clarity of presentation. Individually, each book in this collection represents a milestone in the development of scientific thought and pedagogy; collectively these books amount to an unparalleled scientific library for the enjoyment of a new generation of readers.
Author : E. Marsch
Publisher : Elsevier
Page : 740 pages
File Size : 40,8 Mb
Release : 2016-04-20
Category : Science
ISBN : 9781483287805
The third COSPAR Colloquium entitled Solar Wind Seven was held in Goslar, Germany in September 1991. Twenty-two countries were represented by scientists, many of whom are leading experts in the area of heliospheric physics. The Proceedings reflect current research on solar wind and particularly emphasizes the source regions. The main topics covered encompass Coronal Heating and Solar Wind Acceleration; Large-Scale Structure of the Interplanetary Medium; Minor Ions, Neutrals and Cosmic Rays in the Heliosphere; Kinetic Physics, Waves and Turbulence and finally Heliospheric Dynamic Phenomena.