Computer Science
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993geoae..33...41p&link_type=abstract
Geomagnetizm i Aehronomiya, vol. 33, p. 41
Computer Science
Radiation Belts, Energetic Particles, Magnetic Storms, Crres (Satellite), Magnetospheric Proton Density, Proton Energy, Satellite Observation, Relativistic Electron Beams
Scientific paper
Variations in 5.2-5.4 MeV radiation belt protons during the magnetic storm of March 24-26, 1991 are analyzed using data obtained by the Granat satellite. During the recovery phase (L = 3.7 +/- 0.1), the intensity of 5.2-5.4 MeV protons increased by two orders of magnitude in comparison with that prior to the storm. The maximum achievable value of the L parameter for the Granat orbit was 3.6. Based on CRRES satellite data, a belt of protons with energies from several MeV to tens of MeV and electrons with energies of about 15 MeV, with maxima at L = 2.2-2.6, was formed at the moment of the sudden commencement of the storm of March 24, 1991 over a period of 1 min. A possible interpretation of these phenomena is proposed in terms of the theory of trapped particle drift during sudden impulses.
Chuchkov E. A.
Pavlov N. N.
Tverskaya L. V.
Tverskoj B. A.
No associations
LandOfFree
Variations of energetic particles in the radiation belts during the strong magnetic storm of March 24-26, 1991 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Variations of energetic particles in the radiation belts during the strong magnetic storm of March 24-26, 1991, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variations of energetic particles in the radiation belts during the strong magnetic storm of March 24-26, 1991 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-786275