Rate of proton intensity decay in solar cosmic ray events as a generalized characteristic of the interplanetary space-Reference-Cited by-同舟云学术

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Rate of proton intensity decay in solar cosmic ray events as a generalized characteristic of the interplanetary space

Published:2007-11-20 Issue:3 Volume:7 Page:
ISSN:1524-4423
Container-title:International Journal of Geomagnetism and Aeronomy
language:en
Short-container-title:Int. J. Geomagn. Aeron.

Author:

Daibog E. I.,Logachev Yu. I.,Kecskeméty K.

Publisher

American Geophysical Union (AGU)

Reference20 articles.

1. Invariant spectral characteristics of the decay phases of energetic electron intensities in solar particle events;Daibog;Adv. Space Res.,2000

2. Statistical characteristics of SEP event flux declines through a long period of time (1974–2001);Daibog;Izv. Russ. Akad. Nauk, Ser. Phys.,2003

3. Statistical properties of SEP event flux declines;Daibog;Adv. Space. Res.,2003

4. Relation of SEP event 2–4.6 MeV decline characteristics to solar wind parameters;Daibog;Adv. Space Res.,2005

5. Correlation with parameters of interplanetary space of characteristics of temporal profiles of events in energetic particles during their decline phase;Daibog;Izv. Russ. Akad. Nauk, Ser. Phys.,2005

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Decay phase of energetic electrons and protons in solar cosmic ray events;Bulletin of the Russian Academy of Sciences: Physics;2009-03

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