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Journal of Geophysical Research: Space Physics
Volumn 103, Issue A6, 1998, Pages 12049-12067
Heliospheric tomography using interplanetary scintillation observations 1. Combined Nagoya and Cambridge data
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Indexed keywords

EID: 0001024512     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (183)
References (3)
  • 1
    • 0002635690 scopus 로고
    • Seismic tomography
    • Anderson, D. L., and A. M. Dziewonski, Seismic tomography, Sci. Am., 251(4), 60-68, 1984.
    • (1984) Sci. Am. , vol.251 , Issue.4 , pp. 60-68
    • Anderson, D.L.1    Dziewonski, A.M.2
  • 2
    • 0001335860 scopus 로고
    • Can coronal loop transients be driven magnetically
    • Anzer, U., Can coronal loop transients be driven magnetically, Sol. Phys., 57, 111-118, 1978.
    • (1978) Sol. Phys. , vol.57 , pp. 111-118
    • Anzer, U.1
  • 3
    • 0002859710 scopus 로고    scopus 로고
    • Heliospheric tomography using interplanetary scintillation observations, 3, Correlation between speed and electron density fluctuations in the solar wind
    • Asai, K., M. Kojima, M. Tokumaru, A. Yokobe, B. V. Jackson, P. L. Hick, and P. K. Manhoran, Heliospheric tomography using interplanetary scintillation observations, 3, Correlation between speed and electron density fluctuations in the solar wind, J. Geophys. Res., 103, 1991-2001, 1998.
    • (1998) J. Geophys. Res. , vol.103 , pp. 1991-2001
    • Asai, K.1    Kojima, M.2    Tokumaru, M.3    Yokobe, A.4    Jackson, B.V.5    Hick, P.L.6    Manhoran, P.K.7

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.