What For Does the Sun Need Magnetic Tornadoes?
- Autores: Khabarova O.V1
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Afiliações:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences
- Edição: Nº 1 (2022)
- Páginas: 22-35
- Seção: Articles
- URL: https://journals.eco-vector.com/0044-3948/article/view/628475
- DOI: https://doi.org/10.7868/S0044394822010029
- ID: 628475
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Resumo
Magnetic tornadoes are objects in plasma, which resemble tornadoes in the Earth’s atmosphere, but are observed on the Sun. These structures were discovered almost a century ago, but became a subject for discussions in a last decade only. Improved instruments gave opportunity to observe the details, which are essential to understand the nature of magnetic tornadoes. We discuss the appearance and the behaviour of these objects and the way they are studied.
Sobre autores
O. Khabarova
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences
Bibliografia
- Wedemeyer-Böhm, S. et al. Magnetic tornadoes as energy channels into the solar corona. Nature 486, 505–508 (2012). https://doi.org/10.1038/nature11202
- Xing Li et al. A Solar Tornado Observed by AIA/SDO: Rotational Flow and Evolution of Magnetic Helicity in a Prominence and Cavity, ApJL, 752, L22, (2012). https://doi.org/10.1088/2041-8205/752/2/L22
- Wedemeyer, S. et al. Are Giant Tornadoes the Legs of Solar Prominences? ApJ, 774, 123, (2013). https://doi.org/10.1088/0004-637X/774/2/123
- Khabarova O.V. et al. High-latitude conic current sheets in the solar wind, ApJ, 836, 108, (2017). https://doi.org/10.3847/1538-4357/836/1/108
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