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Volumn 610, Issue 2 II, 2004, Pages

On the temporal relationship between Hα filament eruptions and soft X-ray emissions

Author keywords

Methods: statistical; Stars: flare; Sun: chromosphere; Sun: coronal mass ejections (CMEs); Sun: filaments; Techniques: image processing

Indexed keywords


EID: 4043095615     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/423170     Document Type: Article
Times cited : (14)

References (16)
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    • Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, ed. A. A. Pevtsov & H. Uitenbroek (San Francisco: ASP)
    • Denker, C., Didkovsky, L. V., Marquette, W. H., Goode, P. R., Venkateswaran, K., & Rimmele, T. R. 2003, in ASP Conf. Ser. 286, Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, ed. A. A. Pevtsov & H. Uitenbroek (San Francisco: ASP), 23
    • (2003) ASP Conf. Ser. , vol.286 , pp. 23
    • Denker, C.1    Didkovsky, L.V.2    Marquette, W.H.3    Goode, P.R.4    Venkateswaran, K.5    Rimmele, T.R.6
  • 6
  • 10
    • 5644278535 scopus 로고
    • Royal Observatory, Greenwich. 1930, MNRAS, 91, 239
    • (1930) MNRAS , vol.91 , pp. 239
  • 14
    • 0001623399 scopus 로고
    • ed. M. J. Rycroft & S. K. Runcorn (Berlin: Akademie)
    • Tousey, R. 1973, in Space Research XIII, ed. M. J. Rycroft & S. K. Runcorn (Berlin: Akademie), 713
    • (1973) Space Research XIII , pp. 713
    • Tousey, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.