Machine learning in solar physics

Autor: Andrés Asensio Ramos, Mark C. M. Cheung, Iulia Chifu, Ricardo Gafeira

Publikováno v: Living Reviews in Solar Physics, Vol 20, Iss 1, Pp 1-89 (2023)

Abstract The application of machine learning in solar physics has the potential to greatly enhance our understanding of the complex processes that take place in the atmosphere of the Sun. By using techniques such as deep learning, we are now in the p

Externí odkaz: https://doaj.org/article/97eff4c7739e4050935fbc2ef60a8aea

3D Solar Coronal Loop Reconstructions with Machine Learning

Autor: Iulia Chifu, R. Gafeira

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)

This is an open access article, original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, j

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6be050f67c9c533638e1502710e4b328
http://hdl.handle.net/10261/241356

Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data

Autor: A. De Groof, Marilena Mierla, Bernd Inhester, Andrei Zhukov, Guillermo Stenborg, Iulia Chifu, Daniel B. Seaton, David Berghmans, Luciano Rodriguez

Publikováno v: Solar Physics. 286:241-253

Observations of the early rise and propagation phases of solar eruptive prominences can provide clues about the forces acting on them through the behavior of their acceleration with height. We have analyzed such an event, observed on 13 April 2010 by

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ae1514f59751e68bec9c104ed814a59
https://doi.org/10.1007/s11207-012-9965-0

Low polarized emission from the core of coronal mass ejections

Autor: L. Rodriguez, Bernd Inhester, Iulia Chifu, Andrei Zhukov, Marilena Mierla

In white-light coronagraph images, cool prominence material is sometimes observed as bright patches in the core of coronal mass ejections (CMEs). If, as generally assumed, this emission is caused by Thomson-scattered light from the solar surface, it

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31efe97214a1fbee549d55802da9f59d
http://arxiv.org/abs/1105.3391

Multiwavelengths study of active region 09778

Autor: Iulia Chifu, Oana Chiricuta, Diana Constantin, Cristiana Dumitrache, Vasile Mioc, Nedelia A. Popescu

Publikováno v: AIP Conference Proceedings.

We have studied the evolution and decay of the active region 09778, as well as the evolution of the filament below it and its possible relation with the active region. Using data from SOHO—LASCO, BBSO, Mauna Loa, we analyzed the evolution of active

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::18e1c306a0091a289eef8263e14e67e5
https://doi.org/10.1063/1.2993660