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- W92453957 abstract "Abstract. Spectropolarimetric observations of the internetwork obtained in the 1.56 µm Fedoubletare used to calculate the distributions of magnetic fie ld strength, fillin g factor and magnetic flu x densityat different positions on the solar surface. We go one step further and describe what the observationsshow about the three-dimensional structure of the magnetic fie lds at the internetwork quiet Sun.1 Our knowledge of the magnetic fi eld in the internetwork ... ... has evolved rapidly in recent years. Nowadays, concerning the Zeeman effect, the mostreliable works of internetwork magnetic fi elds deal with the infrared Fedoublet situated at1.56 µm (Khomenko et al. 2003; S´anchez Almeida et al. 2003; Dom´inguez Cerde˜na et al.2006; Mart´inez Gonza´lez et al. 2007) or with spectral lines with hyperfi ne structure. Lop´ ezAriste et al. (2006) use the visible Mnat 553.7 nm and Asensio Ramos et al. (2007) analyzethe Mnline situated at 1.53 µm, in the near infrared part of the spectrum. All these worksare based on spectropolarimetric observations at a spatial resolution of the order of 1" @default.
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- W92453957 date "2007-01-01" @default.
- W92453957 modified "2023-09-23" @default.
- W92453957 title "Internetwork magnetic fi elds" @default.
- W92453957 hasPublicationYear "2007" @default.
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