A Chromatic Treatment of Linear Polarization in the Solar Corona at the 2023 Total Solar Eclipse

The broadband solar K-corona is linearly polarized due to Thomson scattering. Various strategies have been used to represent coronal polarization. Here, we present a new way to visualize the polarized corona, using observations from the 2023 April 20 total solar eclipse in Australia in support of th...

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Veröffentlicht in:	Research notes of the AAS 2023-11, Vol.7 (11), p.241
Hauptverfasser:	Patel, Ritesh, Seaton, Daniel B., Caspi, Amir, Kovac, Sarah A., Davis, Sarah J., Carini, John P., Gardner, Charles H., Gosain, Sanjay, Klein, Viliam, Laatsch, Shawn A., Reiff, Patricia H., Saini, Nikita, Weir, Rachael, Zietlow, Daniel W., Elmore, David F., Ursache, Andrei E., DeForest, Craig E., West, Matthew J., Bruenjes, Fred, Winter, Jen
Format:	Artikel
Sprache:	eng
Schlagworte:	Polarimetry Solar corona Solar eclipses Solar K corona
Online-Zugang:	Volltext
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