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Autor:
Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta, Regina Aznar Cuadrado, Udo Schühle, Luca Teriaca, Sami K. Solanki, Louise Harra, David Berghmans, Frédéric Auchère, Susanna Parenti, Andrei N. Zhukov, Éric Buchlin, Cis Verbeeck, Emil Kraaikamp, Luciano Rodriguez, David M. Long, Conrad Schwanitz, Krzysztof Barczynski, Gabriel Pelouze, Philip J. Smith, Wei Liu, Mark C. Cheung
Publikováno v:
Astronomy & Astrophysics, 670
The solar chromosphere hosts a wide variety of transients, including dynamic fibrils (DFs) that are characterised as elongated, jet-like features seen in active regions, often through Hα diagnostics. So far, these features have been difficult to ide
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8ac531ddfb0209046802cf69f74ecd5
https://hdl.handle.net/20.500.11850/597508
https://hdl.handle.net/20.500.11850/597508