Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7752
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dc.contributor.authorNagaraju, K-
dc.contributor.authorSankarasubramanian, K-
dc.contributor.authorRangarajan, K. E-
dc.date.accessioned2021-06-29T06:58:34Z-
dc.date.available2021-06-29T06:58:34Z-
dc.date.issued2020-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 354, pp. 46 - 52en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2248/7752-
dc.descriptionRestricted Accessen_US
dc.description.abstractMeasurement of magnetic field in this layer is challenging both from point of view of observations and interpretation of the data. We present in this work about spectropolarimetric observations of a pore, simultaneously in Ca ii (CaIR) at 854.2 nm (CaIR) and H α (656.28 nm). The observed region includes a small scale energetic event (SSEE) taking place in the region between the pore and the region which show opposite polarity to that of pore at the photosphere. The energetic event appears to be a progressive reconnection event as shown by the time evolution of the intensity profiles. Closer examination of the intensity profiles from the downflow regions suggest that the height of formation of CaIR is higher than that of Hi α, contrary to the current understanding about their height of formation. Preliminary results on the inversion of Stokes-I and V profiles of CaIR are also presented.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.urihttps://doi.org/10.1017/S1743921320000186-
dc.rights© International Astronomical Union ht-
dc.subjectPhotosphere: Magnetic fielden_US
dc.subjectChromosphere: Magnetic fielden_US
dc.subjectMulti-line-Spectropolarimetryen_US
dc.titleDiagnosing chromospheric magnetic field through simultaneous spectropolarimetry in Hα and Ca II 854.2 nmen_US
dc.typeArticleen_US
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