High energy cosmic-ray nuclei results on Ulysses: 2. Effects of a recurrent high-speed stream from the southern polar coronal hole

Space Science Reviews

Volumn 72, Issue 1-2, 1995, Pages 397-402

  Kunow, H ^a   Droge W ^a   Heber, B ^a   Muller Mellin R ^a   Rohrs K ^a   Sierks, H ^a   Wibberenz, G ^a   Ducros, R ^b   Ferrando, P ^b   Rastoin, C ^b   Raviart, A ^b   Paizis, C ^c  

^a UNIVERSITY OF KIEL   (Germany)

^b CEA SACLAY   (France)

^c UNIVERSITY OF MILAN   (Italy)

Author keywords

Corotating Interaction Region; Heliosphere; solar modulation; Ulysses

Indexed keywords

EID: 0039209992     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/BF00768811     Document Type: Article

References (14)

1. The evolution of the interplanetary sector structure in 1992
2. Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer belt
3. Counterstreaming suprathermal electron events upstream of corotating shocks in the solar wind beyond ∼2 Au: Ulysses
4. Latitudinal variation of solar wind corotating stream interaction regions: Ulysses
5. Disappearance of the heliospheric sector structure at Ulysses