Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of Björn Müller

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Journal Article (2)

1.
Journal Article
Müller, B.; Hohage, T.; Fournier, D.; Gizon, L.: Quantitative passive imaging by iterative holography: the example of helioseismic holography. Inverse Problems 40, p. 045016 (2024)
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2.
Journal Article
Kollatschny, W.; Ochmann, M. W.; Kaspi, S.; Schumacher, C.; Behar, E.; Chelouche, D.; Horne, K.; Müller, B.; Rafter, S. E.; Chini, R. et al.; Haas, M.; Probst, M. A.: The Great Slump: Mrk 926 reveals discrete and varying Balmer line satellite components during a drastic phase of decline. Astronomy and Astrophysics 657, p. A122 (2022)
MPG.PuRe
DOI
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