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Detecting coronal mass ejections with machine learning methods

Published online by Cambridge University Press:  23 December 2024

K. VidaOpen the ORCID record for K. Vida[Opens in a new window],
B. Seli,
T. Szklenár,
L. Kriskovics,
A. GörgeiOpen the ORCID record for A. Görgei[Opens in a new window] and
Zs. Kövári
K. Vida*
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, Hungary
B. Seli
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, Hungary
T. Szklenár
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, Hungary
L. Kriskovics
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, Hungary
A. Görgei
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, HungaryEötvös University, Department of Astronomy, Budapest, Hungary
Zs. Kövári
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, HungaryCSFK, MTA Centre of Excellence, Budapest, Hungary
*
email: vidakris@konkoly.hu
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Abstract

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Flares on the Sun are often associated with ejected plasma: these events are known as coronal mass ejections (CMEs). These events, although are studied in detail on the Sun, have only a few dozen known examples on other stars, mainly detected using the Doppler-shifted absorption/emission features in Balmer lines and tedious manual analysis. We present a possibility to find stellar CMEs with the help of high-resolution solar spectra.

Keywords

Sun: coronal mass ejections (CMEs)Stars: activitymethods: data analysistechniques: spectroscopicNeural networks

Information

Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S365: Dynamics of Solar and Stellar Convection Zones and Atmospheres , December 2023, pp. 404 - 408
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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