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Volumn 462, Issue 3, 2007, Pages 1137-1145

The usefulness of analytic response functions

Author keywords

Line: formation; Magnetic fields; Polarization; Radiative transfer; Sun: magnetic fields; Sun: photosphere

Indexed keywords

FUNCTIONS; HEAT TRANSFER; HIGH ENERGY PHYSICS; LIGHT POLARIZATION; MAGNETIC FIELD MEASUREMENT; SPECTRUM ANALYSIS; SUN; THERMODYNAMICS;

EID: 33846818640     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066201     Document Type: Article
Times cited : (78)

References (19)
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    • High Resolution Solar Physics: Theory, Observations, and Techniques
    • Martínez Pillet, V., Collados, M., Sánchez Almeida, J., et al. 1999, High Resolution Solar Physics: Theory, Observations, and Techniques, ASP Conf. Ser., 183, 264
    • (1999) ASP Conf. Ser , vol.183 , pp. 264
    • Martínez Pillet, V.1    Collados, M.2    Sánchez Almeida, J.3
  • 14
    • 23944499109 scopus 로고    scopus 로고
    • & SDO/HMI Team
    • Scherrer, P. H., & SDO/HMI Team 2002, BAAS, 34, 735
    • (2002) BAAS , vol.34 , pp. 735
    • Scherrer, P.H.1
  • 18
    • 0000225864 scopus 로고
    • Unno, W. 1956, PASJ, 8, 108
    • (1956) PASJ , vol.8 , pp. 108
    • Unno, W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.