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Author : John Keith Hargreaves
Publisher : Cambridge University Press
Page : 440 pages
File Size : 46,6 Mb
Release : 1992
Category : Nature
ISBN : 0521427371
Describes the physical conditions in the upper atmosphere and magnetosphere of the Earth
Author : Yohsuke Kamide,Abraham C.-L. Chian
Publisher : Springer Science & Business Media
Page : 539 pages
File Size : 54,8 Mb
Release : 2007-08-02
Category : Science
ISBN : 9783540463146
As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ?. ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth’s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci?cally the close coupling of di?erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment.
Author : Yohsuke Kamide,Abraham C.-L. Chian
Publisher : Springer
Page : 539 pages
File Size : 49,6 Mb
Release : 2009-09-02
Category : Science
ISBN : 3540831339
As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ?. ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth’s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci?cally the close coupling of di?erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment.
Author : Stephen J. Mangis
Publisher : Unknown
Page : 76 pages
File Size : 52,9 Mb
Release : 1975
Category : Geomagnetism
ISBN : MINN:30000010416612
This report is an introduction to solar-terrestrial phenomena for those with no special background in astrophysics or solar astronomy. Discussions of physics have been kept to a minimum, with emphasis on phenomonology instead. An individual completely unfamiliar with solar events should, after reading this volume, be able to read and understand the SESC Report and Forecast of Solar Geophysical Activity and be able to apply its contents to his particular area of concern. This volume is also intended as a quick reference work for Skylab ATM Principal Investigator Teams to assist them in using the ATM data book. For that reason, a list of abbreviations used in forecasts and observatory reports is included. Subjects discussed are solar structure and processes, solar activity, and solar-terrestrial relations. There is a brief description of the Space Environment Services Center's activities.
Author : Kanya Kusano
Publisher : Springer Nature
Page : 470 pages
File Size : 42,8 Mb
Release : 2023-01-31
Category : Science
ISBN : 9789811977657
Powerful solar explosions, such as flares and coronal mass ejections, greatly disturb the electromagnetic environment around the Earth and the atmosphere. They may even impact various social systems—communications, positioning, electric power supply, aviation and activities in space. Such variations in the space environment, which can influence human activities, are called “space weather.” The space weather disaster caused by a solar explosion is a potential risk in modern society. To reduce and mitigate space weather impacts, it is essential to understand the structure and dynamics of the solar–terrestrial environment and to predict the variations. This book comprehensively describes space weather, from the basics of related sciences to the possible social impacts. It was compiled based on a national research project on solar–terrestrial environment prediction conducted in Japan recently. It consists of four parts: the linkage between space weather and society; the magnetosphere of the Earth and space weather prediction; solar storms and space weather prediction; and long-term prediction of solar cycle activity and climate impacts. Each chapter covers the basics and applications of each area, which helps readers gain a broad understanding of the subject matter throughout the book. In addition, readers are able to select and read the topics they are most interested in. It is especially valuable for undergraduate and graduate students and young researchers studying space weather and related topics, and is further helpful for experts in various industries related to space weather disasters. The translation was done with the help of artificial intelligence (machine translation by the service DeepL.com). The present version has been revised technically and linguistically by the authors in collaboration with a professional translator.
Author : John Keith Hargreaves
Publisher : Unknown
Page : 328 pages
File Size : 49,8 Mb
Release : 1979
Category : Science
ISBN : UCAL:B4164307
Author : Donald J. Williams
Publisher : Unknown
Page : 84 pages
File Size : 47,5 Mb
Release : 1976
Category : Geomagnetism
ISBN : MINN:30000010416638
SELDADS = Space Environment Laboratory Data Acquisition and Display System
Author : H. Wang,Ronglan L. Xu
Publisher : Elsevier
Page : 492 pages
File Size : 49,7 Mb
Release : 2002-11-20
Category : Science
ISBN : 0080441106
The COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) was held in the National Astronomy Observatories of Chinese Academy of Sciences (NAOC) in Beijing, China in September 10-12, 2001. The meeting was focused on five areas of the solar-terrestrial magnetic activity and space environment studies, including study on solar surface magnetism; solar magnetic activity, dynamical response of the heliosphere; space weather prediction; and space environment exploration and monitoring. A hot topic of space research, CMEs, which are widely believed to be the most important phenomenon of the space environment, is discussed in many papers. Other papers show results of observational and theoretical studies toward better understanding of the complicated image of the magnetic coupling between the Sun and the Earth, although little is still known little its physical background. Space weather prediction, which is very important for a modern society expanding into out-space, is another hot topic of space research. However, a long way is still to go to predict exactly when and where a disaster will happen in the space. In that sense, there is much to do for space environment exploration and monitoring. The manuscripts submitted to this Monograph are divided into the following parts: (1) solar surface magnetism, (2) solar magnetic activity, (3) dynamical response of the heliosphere, (4) space environment exploration and monitoring; and (5) space weather prediction. Papers presented in this meeting but not submitted to this Monograph are listed by title as unpublished papers at the end of this book.
Author : A.D.M. Walker
Publisher : CRC Press
Page : 466 pages
File Size : 45,9 Mb
Release : 2019-07-28
Category : Science
ISBN : 9780429525001
Solar-terrestrial physics deals with phenomena in the region of space between the surface of the Sun and the upper atmosphere of the Earth, a region dominated by matter in a plasma state. This area of physics describes processes that generate the solar wind, the physics of geospace and the Earth's magnetosphere, and the interaction of magnetospheri
Author : Bertalan Zieger
Publisher : Unknown
Page : 116 pages
File Size : 49,6 Mb
Release : 1997
Category : Solar activity
ISBN : UOM:39015043145377
Author : David Peter Stern
Publisher : Unknown
Page : 114 pages
File Size : 42,6 Mb
Release : 1978
Category : Solar activity
ISBN : OSU:32435010217776
Author : May-Britt Kallenrode
Publisher : Springer Science & Business Media
Page : 487 pages
File Size : 45,5 Mb
Release : 2013-03-09
Category : Science
ISBN : 9783662099599
Observations and physical concepts are interwoven to give basic explanations of phenomena and also show the limitations in these explanations and identify some fundamental questions. Compared to conventional plasma physics textbooks this book focuses on the concepts relevant in the large-scale space plasmas. It combines basic concepts with current research and new observations in interplanetary space and in the magnetospheres. Graduate students and young researchers starting to work in this special field of science, will find the numerous references to review articles as well as important original papers helpful to orientate themselves in the literature. Emphasis is on energetic particles and their interaction with the plasma as examples for non-thermal phenomena, shocks and their role in particle acceleration as examples for non-linear phenomena. This second edition has been updated and extended. Improvements include: the use of SI units; addition of recent results from SOHO and Ulysses; improved treatment of the magnetosphere as a dynamic phenomenon; text restructured to provide a closer coupling between basic physical concepts and observed complex phenomena.
Author : Roger P. Briggs
Publisher : Unknown
Page : 108 pages
File Size : 51,8 Mb
Release : 1993
Category : Geophysics
ISBN : STANFORD:36105126822043
Author : Donald J. Williams
Publisher : Unknown
Page : 0 pages
File Size : 45,9 Mb
Release : 1976
Category : Real-time data processing
ISBN : OCLC:880012379
Author : Anonim
Publisher : Unknown
Page : 94 pages
File Size : 53,6 Mb
Release : 1996
Category : Astronautics
ISBN : UOM:39015038954502