Three-dimensional modeling of chromospheric spectral lines in a simulated active region

Context. Because of the complex physics that governs the formation of chromospheric lines, interpretation of solar chromospheric observations is difficult. The origin and characteristics of many chromospheric features are, because of this, unresolved.

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Copyright 2020 The European Southern Observatory
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Author Bjørgen, J. P.
Leenaarts, J.
Rempel, Matthias
Cheung, M. C. M.
Danilovic, S.
de la Cruz Rodríguez, J.
Sukhorukov, A. V.
Publisher UCAR/NCAR - Library
Publication Date 2019-11-16T00:00:00
Digital Object Identifier (DOI) Not Assigned
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Topic Category geoscientificInformation
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Metadata Date 2025-07-11T19:24:07.744458
Metadata Record Identifier edu.ucar.opensky::articles:23168
Metadata Language eng; USA
Suggested Citation Bjørgen, J. P., Leenaarts, J., Rempel, Matthias, Cheung, M. C. M., Danilovic, S., de la Cruz Rodríguez, J., Sukhorukov, A. V.. (2019). Three-dimensional modeling of chromospheric spectral lines in a simulated active region. UCAR/NCAR - Library. https://n2t.org/ark:/85065/d7f76gsz. Accessed 31 July 2025.

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