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Inversion of Stokes profiles with systematic effects
Stockholm University, Faculty of Science, Department of Astronomy.
Number of Authors: 4
2016 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 590, A87Article in journal (Refereed) Published
Abstract [en]

Quantitative thermodynamical, dynamical and magnetic properties of the solar and stellar plasmas are obtained by interpreting their emergent non-polarized and polarized spectrum. This inference requires the selection of a set of spectral lines that are particularly sensitive to the physical conditions in the plasma and a suitable parametric model of the solar/stellar atmosphere. Nonlinear inversion codes are then used to fit the model to the observations. However, the presence of systematic effects, like nearby or blended spectral lines, telluric absorption, or incorrect correction of the continuum, among others, can strongly affect the results. We present an extension to current inversion codes that can deal with these effects in a transparent way. The resulting algorithm is very simple and can be applied to any existing inversion code with the addition of a few lines of code as an extra step in each iteration.

Place, publisher, year, edition, pages
2016. Vol. 590, A87
Keyword [en]
Sun: magnetic fields, Sun: atmosphere, line: profiles, methods: data analysis
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-132495DOI: 10.1051/0004-6361/201628387ISI: 000378106800133OAI: oai:DiVA.org:su-132495DiVA: diva2:953208
Available from: 2016-08-17 Created: 2016-08-15 Last updated: 2016-08-17Bibliographically approved

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de la Cruz Rodriguez, Jaime
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ReferencesLink to record
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