R. Brajša, D. Sudar, I. Skokic, A. O. Benz, M. Kuhar, A. Kobelski, S. Wedemeyer, S. M. White, H. -G. Ludwig, M. Temmer, S. H. Saar, C. L. Selhorst
Published 2018-12-18Version 1
In this work we use solar observations with the ALMA radio telescope at the wavelength of 1.21 mm. The aim of the analysis is to improve understanding of the solar chromosphere, a dynamic layer in the solar atmosphere between the photosphere and corona. The study has an observational and a modeling part. In the observational part full-disc solar images are analyzed. Based on a modified FAL atmospheric model, radiation models for various observed solar structures are developed. Finally, the observational and modeling results are compared and discussed.
Comments: 4 pages, presented at The 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, July 29 - Aug 3 2018, Boston / Cambridge, USA
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The locations of SNe Ib/c and their comparison to those of WR stars and GRBs
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