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dc.date.accessioned2020-10-01T18:05:17Z
dc.date.available2020-10-01T18:05:17Z
dc.date.created2020-09-29T14:37:36Z
dc.date.issued2020
dc.identifier.citationBharti, L. Sobha, B. Quintero Noda, Carlos Joshi, C. Pandya, U. . Chromospheric plasma ejection above a pore. Monthly notices of the Royal Astronomical Society. 2020, 493(2), 3036-3044
dc.identifier.urihttp://hdl.handle.net/10852/80197
dc.description.abstractABSTRACT We present high spatial resolution observations of short-lived transients, ribbons and jet-like events above a pore in Ca ii H images where fine structure, like umbral dots, light bridges and penumbral microfilaments, is present in the underlying photosphere. We found that current layers are formed at the edges of the convective fine structure, due to the shear between their horizontal field and the ambient vertical field. High vertical electric current density patches are observed in the photosphere around these events, which indicates the formation of a current sheet at the reconnection site. In the framework of past studies, low altitude reconnection could be the mechanism that produces such events. The reconnection is caused by an opposite polarity field produced by the bending of field lines by convective downflows at the edge of pore fine structure.
dc.languageEN
dc.titleChromospheric plasma ejection above a pore
dc.typeJournal article
dc.creator.authorBharti, L.
dc.creator.authorSobha, B.
dc.creator.authorQuintero Noda, Carlos
dc.creator.authorJoshi, C.
dc.creator.authorPandya, U.
cristin.unitcode185,15,3,40
cristin.unitnameRosseland senter for solfysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1834999
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Monthly notices of the Royal Astronomical Society&rft.volume=493&rft.spage=3036&rft.date=2020
dc.identifier.jtitleMonthly notices of the Royal Astronomical Society
dc.identifier.volume493
dc.identifier.issue2
dc.identifier.startpage3036
dc.identifier.endpage3044
dc.identifier.doihttps://doi.org/10.1093/mnras/staa434
dc.identifier.urnURN:NBN:no-83294
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0035-8711
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/80197/2/staa434.pdf
dc.type.versionPublishedVersion
dc.relation.projectNFR/262622


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