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Volumn 180, Issue 1-2, 1998, Pages 179-191

Using strong solar coronal emission lines as coronal flux proxies

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Indexed keywords


EID: 0032374427     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005059816204     Document Type: Article
Times cited : (2)

References (13)
  • 1
    • 0040762048 scopus 로고
    • R. F. Molina and S. Bowyer (eds.), Pergamon Press, New York
    • Bowyer, S. and Molina, R. F.: 1991, in R. F. Molina and S. Bowyer (eds.), Extreme Ultraviolet Astronomy, Pergamon Press, New York, p. 397.
    • (1991) Extreme Ultraviolet Astronomy , vol.397
    • Bowyer, S.1    Molina, R.F.2
  • 7
    • 0005643150 scopus 로고    scopus 로고
    • S. Bowyer and R. F. Molina (eds.), Kluwer Academic Publishers, Dordrecht, Holland
    • Jordan, C.: 1996, in S. Bowyer and R. F. Molina (eds.), Astrophysics in the Extreme Ultraviolet, Kluwer Academic Publishers, Dordrecht, Holland, p. 81.
    • (1996) Astrophysics in the Extreme Ultraviolet , pp. 81
    • Jordan, C.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.