Dayside and Polar Cap Aurora (Astrophysics and Space Science Library, 270)
ISBN-13:
9781402004476
ISBN-10:
1402004478
Edition:
2002
Author:
Per Even Sandholt, H.C. Carlson, A. Egeland
Publication date:
2002
Publisher:
Springer
Format:
Hardcover
301 pages
Category:
Aerospace
,
Aeronautics & Astronautics
,
Astronomy & Space Science
,
Astrophysics
,
Physics
,
Climatology
,
Earth Sciences
,
Geophysics
,
Rivers
,
Nature & Ecology
,
Molecular Physics
,
Engineering
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Book details
ISBN-13:
9781402004476
ISBN-10:
1402004478
Edition:
2002
Author:
Per Even Sandholt, H.C. Carlson, A. Egeland
Publication date:
2002
Publisher:
Springer
Format:
Hardcover
301 pages
Category:
Aerospace
,
Aeronautics & Astronautics
,
Astronomy & Space Science
,
Astrophysics
,
Physics
,
Climatology
,
Earth Sciences
,
Geophysics
,
Rivers
,
Nature & Ecology
,
Molecular Physics
,
Engineering
Summary
Dayside and Polar Cap Aurora (Astrophysics and Space Science Library, 270) (ISBN-13: 9781402004476 and ISBN-10: 1402004478), written by authors
Per Even Sandholt, H.C. Carlson, A. Egeland, was published by Springer in 2002.
With an overall rating of 3.7 stars, it's a notable title among other
Aerospace
(Aeronautics & Astronautics, Astronomy & Space Science, Astrophysics, Physics, Climatology, Earth Sciences, Geophysics, Rivers, Nature & Ecology, Molecular Physics, Engineering) books. You can easily purchase or rent Dayside and Polar Cap Aurora (Astrophysics and Space Science Library, 270) (Hardcover) from BooksRun,
along with many other new and used
Aerospace
books
and textbooks.
And, if you're looking to sell your copy, our current buyback offer is $0.3.
Description
The auroral emissions in the upper atmosphere of the polar regions of the Earth are evidence of the capture of energetic particles from the Sun, streaming by the Earth as the solar wind. These auroral emissions, then, are a window to outer space, and can provide us with valuable information about electrodynamic coupling processes between the solar wind and the Earth's ionosphere and upper atmosphere. Studying the physics of these phenomena extends our understanding of our plasma universe. Ground-based remote-sensing techniques, able to monitor continuously the variations in the signatures of aurorae, in combination with in-situ satellite and rocket measurements, promise to advance dramatically our understanding of the physical processes taking place at the interface of the atmospheres of the Earth and the Sun. Decoding their complexity brings us closer to reliable prediction of communication environments, especially at high latitudes. This understanding, in turn, will help us resolve problems of communication and navigation across polar regions.
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