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Effect of geomagnetic disturbances and solar wind density on relativistic electrons at geostationary orbit

✍ Scribed by Lyatsky, Wladislaw; Khazanov, George V.


Book ID
118665192
Publisher
American Geophysical Union
Year
2008
Tongue
English
Weight
316 KB
Volume
113
Category
Article
ISSN
0148-0227

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By analyzing observational data, it has been possible to determine quantitative relationships that represent the role of the interaction of fast and slow solar wind (SW) streams in the formation of characteristic SW properties at the Earth's orbit. It is shown that maximum values of magnetic field