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Microstructure of the IMF turbulences at 2.5 AU

โœ Scribed by H. Mavromichalaki; A. Vassilaki; L. Marmatsouri; X. Moussas; J.J. Quenby; E.J. Smith


Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
329 KB
Volume
16
Category
Article
ISSN
0273-1177

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Numerical evaluation of statistical acce
โœ X. Moussas; J. J. Quenby; J. F. Valdes-Galicia ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 852 KB

Numerical integration of particle trajectories is performed to evaluate the statistical acceleration coefficients DTc for 1 to 100 MeV protons in a solar wind corotating interaction region (CIR) seen at 2.5 and 5.0 AU. Acceleration is followed in the solar wind reference frame and is due to random w