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Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units

โœ Scribed by Ruiz, M. E.; Dasso, S.; Matthaeus, W. H.; Weygand, J. M.


Book ID
125369224
Publisher
Springer
Year
2014
Tongue
English
Weight
770 KB
Volume
289
Category
Article
ISSN
0038-0938

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โœ G. Chambe ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 302 KB

The slowly varying component of solar X-rays in the 0.5-3 ~ wavelength range has been studied using data obtained by the satellite Explorer 30 (Solrad 8). The intensity of these X-rays is poorly correlated with the centimeter radio flux, contrary to the good correlation found in the spectral bands 1