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Volumn 14, Issue 4, 1987, Pages 355-358

Field line draping about fast coronal mass ejecta: A source of strong out‐of‐the‐ecliptic interplanetary magnetic fields

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Indexed keywords


EID: 84989571899     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL014i004p00355     Document Type: Article
Times cited : (130)

References (29)
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    • Interplanetary shock waves and the structure of solar wind disturbances, C. P. Sonett, P. J. Coleman, J. M. Wilcox, NASA SP‐308, Washington, D.C
    • (1972) Solar Wind , pp. 393-417
    • Hundhausen, A.J.1
  • 21
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    • Mapping the magnetosheath field between the magnetopause and the bow shock: Implications for magnetospheric particle leakage
    • (1984) J. Geophys. Res. , vol.89 , pp. 6829-6834
    • Luhmann, J.G.1
  • 27
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    • Substorm associated traveling compression regions in the distant tail: ISEE‐3 geotail observations
    • (1984) Geophys. Res. Lett. , vol.11 , pp. 657-660
    • Slavin, J.A.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.