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Volumn 29, Issue 12, 2002, Pages 1933-1940

How much of the solar irradiance variations is caused by the magnetic field at the solar surface?

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; MAGNETOMETERS; SOLAR RADIATION;

EID: 0036602068     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(02)00238-7     Document Type: Article
Times cited : (22)

References (32)
  • 10
    • 0025198380 scopus 로고
    • An empirical model of total solar irradiance variations between 1874 and 1988
    • (1990) Science , vol.247 , pp. 556-558
    • Foukal, P.1    Lean, J.2
  • 22
    • 0000624426 scopus 로고
    • The dynamical oscillation and propulsion of magnetic fields in the convective zone of a star. I. General considerations
    • (1987) Astrophys. J , vol.312 , pp. 868-879
    • Parker, E.N.1
  • 23
    • 11944249188 scopus 로고
    • Theoretical properties of Ω-loops in the convective zone of the sun. II. The origin of enhanced solar irradiance
    • (1995) Astrophys. J , vol.440 , pp. 415-420
    • Parker, E.N.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.