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Handbook of the solar-terrestrial environment (Record no. 567134)

MARC details
000 -LEADER
fixed length control field 02764 a2200229 4500
003 - CONTROL NUMBER IDENTIFIER
control field OSt
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
ISBN 9783540463146
040 ## - CATALOGING SOURCE
Transcribing agency IIT Kanpur
041 ## - LANGUAGE CODE
Language code of text/sound track or separate title eng
082 ## - DEWEY DECIMAL CLASSIFICATION NUMBER
Classification number 520
Item number H191
245 ## - TITLE STATEMENT
Title Handbook of the solar-terrestrial environment
Statement of responsibility, etc edited by Yohsuke Kamide and Abraham C. -L. Chian
260 ## - PUBLICATION, DISTRIBUTION, ETC. (IMPRINT)
Name of publisher Springer
Year of publication 2007
Place of publication Berlin
300 ## - PHYSICAL DESCRIPTION
Number of Pages xiv, 539 p
520 ## - SUMMARY, ETC.
Summary, etc <br/>An Overview of the Solar–Terrestrial Environment -- An Overview of the Solar–Terrestrial Environment -- The Sun -- The Solar Interior – Radial Structure, Rotation, Solar Activity Cycle -- Solar Atmosphere -- Solar Wind -- Coronal Mass Ejection -- Solar Radio Emissions -- The Earth -- Magnetosphere -- Ionosphere -- Thermosphere -- Space Plasmas -- Space Plasmas -- Magnetic Reconnection -- Nonlinear Processes in Space Plasmas -- Processes in the Solar-Terrestrial Environment -- The Aurora -- Geomagnetic Storms -- Substorms -- Ultra Low Frequency Waves in the Magnetosphere -- Space Weather -- Effects of the Solar Cycle on the Earth’s Atmosphere -- Planets and Comets in the Solar System -- Planetary Magnetospheres -- The Solar-Comet Interactions.<br/><br/>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.<br/>
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical Term Atmospheric sciences
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical Term Astronomy
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical Term Space sciences
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical Term Astronomy, Observations and Techniques
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Kamide, Yohsuke
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name Chian, Abraham C. -L.
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Koha item type Books
Holdings
Withdrawn status Lost status Damaged status Not for loan Collection code Home library Current library Date acquired Source of acquisition Cost, normal purchase price Full call number Accession Number Cost, replacement price Koha item type
        General Stacks PK Kelkar Library, IIT Kanpur PK Kelkar Library, IIT Kanpur 06/01/2025 7 10848.93 520 H191 A186705 18705.06 Books

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