Magnetic clouds and interplanetary particle transport: A numerical model

Journal of Atmospheric and Solar-Terrestrial Physics

Volumn 64, Issue 18, 2002, Pages 1973-1978

  Kallenrode, May Britt ^a  

^a UNIVERSITY OF OSNABRÜCK   (Germany)

Author keywords

Energetic particles; Interplanetary medium; Magnetic clouds; Particle propagation

Indexed keywords

ASTROPHYSICS; NUMERICAL MODEL;

EID: 0036883510     PISSN: 13646826     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1364-6826(02)00195-5     Document Type: Article

References (16)

1. Recent work on modeling the global field line topology of interplanetary magnetic clouds
2. The temporal and spatial development of MeV proton acceleration at interplanetary shocks
3. Shock as a black box II: Effects of adiabatic deceleration and convection included
4. Rogue SEP events: Modeling
5. Propagation of particles injected from interplanetary shocks: A black box model and its consequences for acceleration theory and data interpretation
6. Energetic particle events: Efficiency of interplanetary shocks as 50 kev < E < 100 MeV protons accelerators
7. Adiabatic Fermi acceleration of energetic particles between converging interplanetary shock waves
8. Using energetic particles to probe the magnetic topology of ejecta
9. Effect of adiabatic deceleration on the focused transport of solar cosmic rays
10. Simulation of magnetic cloud propagation in the inner heliosphere in two-dimensions, 2, a loop parallel to the ecliptic plane and the role of helicity
11. Drapery of IMF around magnetic clouds of different geometry