A new class of forward‐reverse shock pairs in the solar wind

Geophysical Research Letters

Volumn 21, Issue 21, 1994, Pages 2271-2274

  Gosling, J T ^a   McComas, D J ^a   Phillips, J L ^a   Weiss, L A ^a   Pizzo, V J ^a   Goldstein, B E ^a   Forsyth, R J ^a  

^a NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001280957     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/94GL02245     Document Type: Article

References (15)

1. The magnetic field investigation on the Ulysses mission: Instrumentation and preliminary scientific results
2. The Ulysses solar wind plasma experiment
3. Magnetic clouds
4. Coronal mass ejections and magnetic flux ropes in interplanetary space
5. Forward‐reverse shock pairs associated with transient disturbances in the solar wind at 1 AU
6. Counterstreaming suprathermal electron events upstream of corotating shocks in the solar wind beyond ˜2 AU: Ulysses
7. A forward‐reverse shock pair in the solar wind driven by over‐expansion of a coronal mass ejection: Ulysses observations
8. The speeds of coronal mass ejections in the solar wind at mid heliographic latitudes: Ulysses
9. Some macroscopic properties of shock waves in the heliosphere
10. Numerical simulation of flare‐generated disturbances in the solar wind
11. Solar wind structure at large heliocentric distances: An interpretation of Pioneer 10 observations
12. The speeds of coronal mass ejections: SMM observations from 1980 and 1984–1989
13. Ulysses at 50° south: Constant immersion in the high‐speed solar wind
14. Interplanetary shocks on the large scale: A retrospective on the last decade's theoretical efforts
15. Observations of interaction regions and corotating shocks between one and five AU: Pioneers 10 and 11