메뉴 건너뛰기




Volumn 493, Issue 2 PART II, 1998, Pages

Self-consistent and time-dependent magnetohydrodynamic chromosphere models for magnetically active stars

Author keywords

MHD; Stars: activity; Stars: chromospheres; Stars: late type; Stars: rotation

Indexed keywords


EID: 22444453775     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/311130     Document Type: Article
Times cited : (28)

References (31)
  • 12
    • 0002173535 scopus 로고    scopus 로고
    • _. 1996, Space Sci. Rev., 75, 453
    • (1996) Space Sci. Rev. , vol.75 , pp. 453
  • 17
    • 0010745890 scopus 로고
    • Rutten, R. G. M. 1986, A&A, 159, 291
    • (1986) A&A , vol.159 , pp. 291
    • Rutten, R.G.M.1
  • 18
    • 0001619480 scopus 로고
    • _. 1987, A&A, 177, 131
    • (1987) A&A , vol.177 , pp. 131
  • 20
    • 0040467443 scopus 로고    scopus 로고
    • Magnetodynamic Phenomena in the Solar Atmosphere - Prototypes of Stellar Magnetic Activity, ed. Y. Uchida et al. (Dordrecht: Kluwer)
    • Saar, S. H. 1996, in IAU Colloq. 153, Magnetodynamic Phenomena in the Solar Atmosphere - Prototypes of Stellar Magnetic Activity, ed. Y. Uchida et al. (Dordrecht: Kluwer), 367
    • (1996) IAU Colloq. , vol.153 , pp. 367
    • Saar, S.H.1
  • 23
  • 26
    • 0005792575 scopus 로고    scopus 로고
    • Stellar Surface Structure, ed. K. G. Strassmeier & J. L. Linsky (Dordrecht: Kluwer)
    • Solanki, S. K. 1996, in IAU Symp. 176, Stellar Surface Structure, ed. K. G. Strassmeier & J. L. Linsky (Dordrecht: Kluwer), 201
    • (1996) IAU Symp. , vol.176 , pp. 201
    • Solanki, S.K.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.