The Solar wind and the earth
Author(s)
Bibliographic Information
The Solar wind and the earth
（Geophysics and astrophysics monographs）
Terra Scientific Pub. , D. Reidel, c1987
- : pbk.
Available at / 24 libraries
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Institute for Space–Earth Environmental Research, Nagoya University宇宙地球研1
444||Ak||||太陽図書室41068946
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Note
Includes bibliographies and index
Description and Table of Contents
- Volume
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ISBN 9789027724717
Description
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.
Table of Contents
1 The Sun's Spots and Flares.- 2 Solar Wind and Heliosphere.- 3 Cosmic Rays and Energetic Particles in the Heliosphere.- 4 The Earth as a Magnet.- 5 The Magnetosphere.- 6 Plasma Populations in the Magnetosphere.- 7 The Ionosphere.- 8 The Aurora.- 9 The Role of Magnetospheric Substorms in Magnetosphere-Ionosphere Coupling.- 10 Plasma Wave Phenomena in the Earth's Magnetosphere.- 11 Active Plasma Experiments.- 12 The Earth's Thermosphere.- 13 Ozone and the Stratosphere.- 14 Solar Power Satellites.
- Volume
-
: pbk. ISBN 9789027724724
Description
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.
Table of Contents
1 The Sun's Spots and Flares.- 2 Solar Wind and Heliosphere.- 3 Cosmic Rays and Energetic Particles in the Heliosphere.- 4 The Earth as a Magnet.- 5 The Magnetosphere.- 6 Plasma Populations in the Magnetosphere.- 7 The Ionosphere.- 8 The Aurora.- 9 The Role of Magnetospheric Substorms in Magnetosphere-Ionosphere Coupling.- 10 Plasma Wave Phenomena in the Earth's Magnetosphere.- 11 Active Plasma Experiments.- 12 The Earth's Thermosphere.- 13 Ozone and the Stratosphere.- 14 Solar Power Satellites.
by "Nielsen BookData"