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Volumn 29, Issue 9, 2002, Pages 42-1-42-4

Factors controlling the location of the Bow Shock at Mars

Author keywords

[No Author keywords available]

Indexed keywords

ELECTRIC FIELD EFFECTS; MAGNETOMETERS; ORBITS; REFLECTOMETERS; SPACECRAFT;

EID: 0036558533     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001gl014513     Document Type: Article
Times cited : (53)

References (19)
  • 2
    • 17744416393 scopus 로고    scopus 로고
    • Global distribution of crustal magnetization discovered by the Mars global surveyor MAG/ER experiment
    • (1999) Science , vol.284 , pp. 790-793
    • Acuna, M.H.1
  • 10
    • 2142833267 scopus 로고
    • A statistical study of ions and magnetic field in the Venus magnetotail
    • (1990) J. Geophys. Res , vol.95 , pp. 12005-12018
    • Moore, K.R.1
  • 11
  • 13
    • 0000771297 scopus 로고
    • The Martian magnetic field environment: Induced or dominated by an intrinsic magnetic field
    • (1992) Adv. Space Res , vol.12 , pp. 9213-9219
    • Schwingenschuh, K.1
  • 14
    • 0001148503 scopus 로고
    • The solar wind interaction with Mars: Mariner 4, Mars 2, Mars 3, Mars 5 and Phobos 2 observations of bow shock position and shape
    • (1991) J. Geophys. Res , vol.96 , pp. 11235-11241
    • Slavin, J.A.1
  • 15
    • 0000820734 scopus 로고
    • Plasma wave system measurements of the Martian bow shock from the Phobos 2 spacecraft
    • (1991) J. Geophys. Res , vol.96 , pp. 11253-11264
    • Trotignon, J.G.1
  • 16
  • 17
    • 0034352563 scopus 로고    scopus 로고
    • The solar wind interaction with Mars: Locations and shapes of the bow shock and the magnetic pile-up boundary from the observations of the MAG/ER experiment onboard mars global surveyor
    • (2000) Geophys. Res. Lett , vol.27 , pp. 49-52
    • Vignes, D.1
  • 19
    • 0005028103 scopus 로고
    • Interplanetary magnetic field control of the Mars bow shock: Evidence for Venus like interaction
    • (1991) J. Geophys. Res , vol.96 , pp. 11265-11269
    • Zhang, T.L.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.