Photospheric magnetic field and chromospheric emission

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dc.creatorRezaei, R.
dc.creatorSchlichenmaier, R.
dc.creatorBeck, C.
dc.creatorSchmidt, W.
dc.date2007-01-24
dc.date.accessioned2026-07-07T07:42:43Z
dc.date.available2026-07-07T07:42:43Z
dc.descriptionWe present a statistical analysis of network and internetwork properties in the photosphere and the chromosphere. For the first time we simultaneously observed (a) the four Stokes parameters of the photospheric iron line pair at 630.2 nm and (b) the intensity profile of the Ca II H line at 396.8 nm. The vector magnetic field was inferred from the inversion of the iron lines. We aim at an understanding of the coupling between photospheric magnetic field and chromospheric emission.
dc.description4 pages, appeared in "Modern Solar Facilities: Advanced Solar Sciences", Eds. F. Kneer, K.G. Puschmann, A.D.Wittmann, Sep. 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0701681
dc.identifierhttp://arxiv.org/abs/astro-ph/0701681
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122547
dc.subjectAstrophysics
dc.titlePhotospheric magnetic field and chromospheric emission
dc.typetext

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