2007/01/24 by R. Rezaei, R. Schlichenmaier, Rezaei, R. +5
Biochemistry, Genetics and Molecular Biology · Neuroscience · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Fractal and DNA sequence analysis #Photoreceptor and optogenetics research #Scientific Research and Discoveries #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0701681
4 pages, appeared in "Modern Solar Facilities: Advanced Solar Sciences", Eds. F. Kneer, K.G. Puschmann, A.D.Wittmann, Sep. 2006
arxiv created 2007/01/24 · openalex publication_date 2007/01/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We 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.