Handbook of the Solar-Terrestrial Environment

Abraham C. -L. Chian

ISBN 10: 3642079687 / ISBN 13: 9783642079689

Published by Springer Berlin Heidelberg, 2010

About this Item

Druck auf Anfrage Neuware - Printed after ordering - 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.

Seller Inventory # 9783642079689

Bibliographic Details

• Title: Handbook of the Solar-Terrestrial Environment
• Publisher: Springer Berlin Heidelberg
• Publication Date: 2010
• Language: English
• ISBN 10: 3642079687
• ISBN 13: 9783642079689
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 246W x 189H x 30D millimeters 246 millimeters width by 189 millimeters height by 30 millimeters depth
• Weight: 1062 grams

About this title

Synopsis

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.

Review

From the reviews:

"The book is a solid, comprehensive ... text providing a full overview of solar-terrestrial science, pitched at the graduate student level. The book provides an excellent summary of the underlying physics controlling Sun-Earth connections, and it certainly merits a place on the bookshelf of an academic working in the field. ... is worthwhile for working solar-terrestrial physicists ... . If you are an ambitious graduate student and have decided you want to make a career in solar-terrestrial physics, then you might consider it ... ." (Andy Breen, EOS, Vol. 90 (11), March, 2009)