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Title: Sustained Heating of the Chromosphere and Transition Region Over a Sunspot Light Bridge
Abstract

Sunspot light bridges (LBs) exhibit a wide range of short-lived phenomena in the chromosphere and transition region. In contrast, we use here data from the Multi-Application Solar Telescope (MAST), the Interface Region Imaging Spectrograph (IRIS), Hinode, the Atmospheric Imaging Assembly (AIA), and the Helioseismic and Magnetic Imager (HMI) to analyze the sustained heating over days in an LB in a regular sunspot. Chromospheric temperatures were retrieved from the MAST Caiiand IRIS Mgiilines by nonlocal thermodynamic equilibrium inversions. Line widths, Doppler shifts, and intensities were derived from the IRIS lines using Gaussian fits. Coronal temperatures were estimated through the differential emission measure, while the coronal magnetic field was obtained from an extrapolation of the HMI vector field. At the photosphere, the LB exhibits a granular morphology with field strengths of about 400 G and no significant electric currents. The sunspot does not fragment, and the LB remains stable for several days. The chromospheric temperature, IRIS line intensities and widths, and AIA 171 and 211 Å intensities are all enhanced in the LB with temperatures from 8000 K to 2.5 MK. Photospheric plasma motions remain small, while the chromosphere and transition region indicate predominantly redshifts of 5–20 km s−1with occasional supersonic more » downflows exceeding 100 km s−1. The excess thermal energy over the LB is about 3.2 × 1026erg and matches the radiative losses. It could be supplied by magnetic flux loss of the sunspot (7.5 × 1027erg), kinetic energy from the increase in the LB width (4 × 1028erg), or freefall of mass along the coronal loops (6.3 × 1026erg).

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Authors:
; ; ; ;
Publication Date:
NSF-PAR ID:
10390909
Journal Name:
The Astrophysical Journal
Volume:
942
Issue:
2
Page Range or eLocation-ID:
Article No. 62
ISSN:
0004-637X
Publisher:
DOI PREFIX: 10.3847
Sponsoring Org:
National Science Foundation
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