The structure and evolution of interplanetary shocks and the relevance for particle acceleration

Nuclear Physics B (Proceedings Supplements)

Volumn 39, Issue 1, 1995, Pages 35-44

  Cane, H V ^a,b  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b UNIVERSITY OF TASMANIA   (Australia)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 21844526684     PISSN: 09205632     EISSN: None     Source Type: Journal    
DOI: 10.1016/0920-5632(95)00005-T     Document Type: Article

References (42)

1. Cosmic-ray propagation processes: 2. The energetic storm-particle event
2. Explorer 12 observations of solar cosmic rays and energetic storm particles after the solar flare of September 28, 1961
3. Solar flare shocks in interplanetary space and solar flare particle events
4. The role of interplanetary shocks in the longitude distribution of solar energetic particles
5. Solar Wind
6. An analysis of shock wave disturbances observed at 1 AU from 1971 through 1978
7. The large-scale structure of flare-associated interplanetary shocks
8. Signatures of shock drivers in the solar wind and their dependence on the solar source location
9. Solar Wind Five
10. The cosmic ray flare effect
11. Energetic interplanetary shocks, radio emission, and coronal mass ejections
12. Activity associated with the solar origin of coronal mass ejections
13. Proc. Solar Wind 6
14. Proc. Solar Wind 6
15. Type II solar radio bursts, interplanetary shocks, and energetic particle events
16. Collisionless Shocks in the Heliosphere: Reviews of current Research
17. Dependence of auroral middle UV emissions on the incident electron spectrum and neutral atmosphere
18. Satellite observations of interplanetary shock waves
19. Energetic particle observations at the Helios 1 spacecraft of shocks associated with coronal mass ejections
20. Proc. 26th ESLAB Symp.
21. Cosmic ray decreases and particle acceleration in 1978-1982 and the associated solar wind structures
22. Solar filament eruptions and energetic particle events
23. Interplanetary ions during an energetic storm particle event: The distribution function from solar wind thermal energies to 1.6 MeV
24. Collisionless Shocks in the Heliosphere: Reviews of current Research