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dc.date.accessioned2021-11-25T18:26:51Z
dc.date.available2021-11-25T18:26:51Z
dc.date.created2021-11-13T16:50:14Z
dc.date.issued2021
dc.identifier.citationFelipe, Tobias de Jorge Henriques, Vasco Manuel de la Cruz Rodriguez, Jaime Socas-Navarro, Hector . Downflowing umbral flashes as evidence of standing waves in sunspot umbrae. Astronomy and Astrophysics (A & A). 2021, 645
dc.identifier.urihttp://hdl.handle.net/10852/89330
dc.description.abstractContext. Umbral flashes are sudden brightenings commonly visible in the core of some chromospheric lines. Theoretical and numerical modeling suggests that they are produced by the propagation of shock waves. According to these models and early observations, umbral flashes are associated with upflows. However, recent studies have reported umbral flashes in downflowing atmospheres. Aims. We aim to understand the origin of downflowing umbral flashes. We explore how the existence of standing waves in the umbral chromosphere impacts the generation of flashed profiles. Methods. We performed numerical simulations of wave propagation in a sunspot umbra with the code MANCHA. The Stokes profiles of the Ca  II 8542 Å line were synthesized with the NICOLE code. Results. For freely propagating waves, the chromospheric temperature enhancements of the oscillations are in phase with velocity upflows. In this case, the intensity core of the Ca  II 8542 Å atmosphere is heated during the upflowing stage of the oscillation. However, a different scenario with a resonant cavity produced by the sharp temperature gradient of the transition region leads to chromospheric standing oscillations. In this situation, temperature fluctuations are shifted backward and temperature enhancements partially coincide with the downflowing stage of the oscillation. In umbral flash events produced by standing oscillations, the reversal of the emission feature is produced when the oscillation is downflowing. The chromospheric temperature keeps increasing while the atmosphere is changing from a downflow to an upflow. During the appearance of flashed Ca  II 8542 Å cores, the atmosphere is upflowing most of the time, and only 38% of the flashed profiles are associated with downflows. Conclusions. We find a scenario that remarkably explains the recent empirical findings of downflowing umbral flashes as a natural consequence of the presence of standing oscillations above sunspot umbrae.
dc.languageEN
dc.titleDownflowing umbral flashes as evidence of standing waves in sunspot umbrae
dc.typeJournal article
dc.creator.authorFelipe, Tobias
dc.creator.authorde Jorge Henriques, Vasco Manuel
dc.creator.authorde la Cruz Rodriguez, Jaime
dc.creator.authorSocas-Navarro, Hector
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1954286
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy and Astrophysics (A & A)&rft.volume=645&rft.spage=&rft.date=2021
dc.identifier.jtitleAstronomy and Astrophysics (A & A)
dc.identifier.volume645
dc.identifier.pagecount7
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202039966
dc.identifier.urnURN:NBN:no-91936
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-6361
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/89330/1/aa39966-20.pdf
dc.type.versionPublishedVersion
cristin.articleidL12
dc.relation.projectEC/H2020/682462
dc.relation.projectNFR/262622


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