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Volumn 100, Issue 1-2, 1985, Pages 415-434

Modern observations of solar prominences

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EID: 0001493083     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/BF00158439     Document Type: Article
Times cited : (124)

References (96)
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  • 5
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    • Bommier, V., Leroy, J. L., and Sahal-Bréchot, S.: 1985b, in M. J. Hagyard (ed.), Measurements of Solar Magnetic Fields, NASA Conf. Publ. CP-2374, p. 375.
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    • Jensen, E., Maltby, P., and Orrall, F. Q. (eds.): 1979, ‘Physics of Solar Prominences’, IAU Colloq.44.
  • 41
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    • Kubota, J.: 1980, in F. Moriyama and J. C. Henoux (eds.) Proc. Japan-France Seminar on Solar Physics, p. 178.
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    • Physical conditions in the cool parts of prominences. III The Sr(+)/Ba(+) resonance line ratios and the internal Lyman-alpha flux
    • (1985) The Astrophysical Journal , vol.290 , pp. 369
    • Landman, D.A.1
  • 49
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    • Leroy, J. L.: 1985, in M. J. Hagyard (ed.), Measurements of Solar Magnetic Fields, NASA Conf. Publ. CP-2374, p. 121.
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    • Morishita, H.: 1985, Tokyo Astron. Bull. 2nd Ser., No. 272, 3123.
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    • Rust, D. M.: 1972, AFCRL-72-0048 (Sacramento Peak Observatory Project 7649).
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    • Uchida, U. and Shibata, K.: 1985, Solar Phys. (submitted).
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    • Two-dimensional nonlocal thermodynamic equilibrium transfer computations of resonance lines in quiescent prominences
    • (1982) The Astrophysical Journal , vol.254 , pp. 780
    • Vial, J.C.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.