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Volumn 506, Issue 3, 2009, Pages 1415-1428

The quiet Sun magnetic field observed with ZIMPOL on THEMIS

Author keywords

Magnetic fields; Methods: data analysis; Polarization; Sun: magnetic fields; Techniques: polarimetric; Turbulence

Indexed keywords

COMPLEX MEDIUM; DIRECT DETERMINATION; FIELD DETERMINATION; FIELD STRENGTHS; FILLING FACTOR; INVERSION CODE; INVERSION RESULTS; LOCAL AVERAGE; MAGNETIC FIELD STRENGTHS; MAGNETIC FIELD VECTORS; MAGNETIC FILLINGS; MEAN MAGNETIC FIELD; METHODS: DATA ANALYSIS; POLARIMETRIC DATA; PROBABILITY DENSITY FUNCTION (PDF); QUIET SUN; STATISTICAL DESCRIPTIONS; SUN: MAGNETIC FIELDS; TECHNIQUES: POLARIMETRIC; ZEEMAN EFFECT;

EID: 70350774357     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811373     Document Type: Article
Times cited : (27)

References (44)
  • 41
    • 0038659611 scopus 로고    scopus 로고
    • Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST
    • Stenflo, J. O., & Holzreuter, R. 2003, Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, ASP Conf. Ser., 286, 169
    • (2003) ASP Conf. Ser. , vol.286 , pp. 169
    • Stenflo, J.O.1    Holzreuter, R.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.