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Volumn 20, Issue 1, 1997, Pages 115-120

Modeling the interplanetary propagation of 0.1-20 MeV shock-accelerated protons. I: Effects of the adiabatic deceleration and solar wind convection

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EID: 0042724150     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00492-4     Document Type: Article
Times cited : (5)

References (11)
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  • 2
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  • 3
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    • A numerical study of the pitch-angle scattering of cosmic rays
    • Kóta, J., E. Merényi, J.R. Jokipii, D.A. Kopriva, T. Gombosi, et al., A numerical study of the pitch-angle scattering of cosmic rays, ApJ, 254, 398 (1982).
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    • Kóta, J.1    Merényi, E.2    Jokipii, J.R.3    Kopriva, D.A.4    Gombosi, T.5
  • 6
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    • Modeling the interplanetary propagation of 0.1-20 MeV shock-accelerated protons. II: Evolution of the injection rate in long-lasting ESP events
    • this issue
    • Lario D., B. Sanahuja, and A.M. Heras, Modeling the interplanetary propagation of 0.1-20 MeV shock-accelerated protons. II: Evolution of the injection rate in long-lasting ESP events, Adv. Space Res., this issue (1996).
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    • Ruffolo, D.1
  • 9
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    • Observations of three-dimensional anisotropies of 35-1000 keV protons associated with interplanetary shocks
    • Sanderson, T.R., R. Reinhard, P. van Nes, and K.-P. Wenzel, Observations of three-dimensional anisotropies of 35-1000 keV protons associated with interplanetary shocks J. Geophys. Res., 90, 19 (1985).
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.