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

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

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..115l&link_type=abstract

Advances in Space Research, vol. 20, p. 115

Astronomy and Astrophysics

Astronomy

3

Interplanetary Space, Shock Wave Propagation, Solar Wind Velocity, Solar Protons, Particle Acceleration, Solar Convection (Astronomy), Astronomical Models, Deceleration, Adiabatic Conditions, Particle Flux Density, Magnetic Storms

Scientific paper

A numerical code is presented that encompasses adiabatic deceleration
and solar wind convection effects. The code is applied to various
validating cases, and the influence of the two effects on the flux and
anisotropy profiles of energetic storm particle events is discussed.

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