Diagnosing chromospheric magnetic field through simultaneous spectropolarimetry in Hα and Ca II 854.2 nm
Abstract
Measurement 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.
- Publication:
-
Solar and Stellar Magnetic Fields: Origins and Manifestations
- Pub Date:
- 2020
- DOI:
- 10.1017/S1743921320000186
- Bibcode:
- 2020IAUS..354...46N
- Keywords:
-
- Photosphere: Magnetic field;
- Chromosphere: Magnetic field;
- Multi-line-Spectropolarimetry