Excess heating of4He2+ and O6+ relative to H+ downstream of interplanetary shocks

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A2, 1997, Pages 2623-2635

  Berdichevsky, Daniel ^a,e   Geiss, Johannes ^b   Gloeckler, George ^c   Mall, Urs ^d  

^a HUGHES STX CORPORATION   (United States)

^b UNIVERSITY OF BERN   (Switzerland)

^c UNIVERSITY OF MARYLAND   (United States)

^d UNIVERSITY OF MICHIGAN   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149043823     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JA02541     Document Type: Article

References (5)

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3. Balogh, A., R.J. Forsyth, A. Ahuja, D.J. Southwood, E.J. Smith, and B.T. Tsurutani, The interplanetary magnetic field from 1 to 5 AU: Ulysses, Adv. Space Res., 13, (6) 15-(6)24, 1993.
4. Balogh, A., J. Gonzalez-Esparza, R. Forsyth, M. Burton, B. Goldstein, E.J. Smith, and S. Bame, Interplanetary shock waves: Ulysses observations in and out of the ecliptic plane, Space Sci. Rev., 72, 171-180, 1995.
5. Baring, M., K. Ogilvie, D. Ellison, and R. Forsyth, Acceleration of solar wind ions by oblique interplanetary shocks, Adv. Space Res., 15, 385-388, 1995.