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Chromospheric Magnetic Fields: Observations, Simulations and their Interpretation
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy.
2012 (English)In: SECOND ATST-EAST MEETING: MAGNETIC FIELDS FROM THE PHOTOSPHERE TO THE CORONA, SAN FRANCISCO: ASTRONOMICAL SOC PACIFIC , 2012, Vol. 463, 15-23 p.Conference paper, Published paper (Refereed)
Abstract [en]

The magnetic field of the quiet-Sun chromosphere remains a mystery for solar physicists. The reduced number of chromospheric lines are intrinsically hard to model and only a few of them are magnetically sensitive. In this work, we use a 3D numerical simulation of the outer layers of the solar atmosphere, to asses the reliability of non-LTE inversions, in this case applied to the Ca II lambda 8542 angstrom line. We show that NLTE inversions provide realistic estimates of physical quantities from synthetic observations.

Place, publisher, year, edition, pages
SAN FRANCISCO: ASTRONOMICAL SOC PACIFIC , 2012. Vol. 463, 15-23 p.
Series
Astronomical Society of the Pacific Conference Series, 463
National Category
Natural Sciences
Identifiers
URN: urn:nbn:se:uu:diva-197227ISI: 000314795500002OAI: oai:DiVA.org:uu-197227DiVA: diva2:612011
Conference
2nd ATST-EAST workshop in Solar Physics, nov 09-11, 2011, Washington, DC
Available from: 2013-03-19 Created: 2013-03-19 Last updated: 2013-03-19Bibliographically approved

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de la Cruz Rodriguez, Jaime

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