Small-scale chromospheric jets above a sunspot light bridge

Abstract

High-resolution broadband filtergrams of active region NOAA 11271 in Ca ii H and G band were obtained with the Solar Optical Telescope on board Hinode to identify the physical driver responsible for the dynamic and small-scale chromospheric jets above a sunspot light bridge. We identified the jets in the Ca images using a semi-automatic routine. The chromospheric jets consist of a bright, triangular-shaped blob that lies on the light bridge, while the apex of this blob extends into a spike-like structure that is bright against the dark umbral background. Most of the jets have apparent lengths of less than 1000 km and about 30% of them have lengths between 1000-1600 km. They are oriented within +/-35 deg. to the normal of the light bridge axis. Many of them are clustered near the central part within a 2 arcsec area. The jets are seen to move rapidly along the light bridge and most of them cannot be identified in successive images taken with a 2 min cadence. The jets are primarily located on one side of the light bridge and are directed into the umbral core. The Stokes profiles at or close to the location of the blobs on the LB exhibit both a significant net circular polarization and multiple components, including opposite-polarity lobes. The magnetic field diverges from the light bridge towards the umbral cores that it separates. In the photosphere there is a predominantly uni-directional flow with speeds of 100-150 m/s along the light bridge which is interrupted by a patch of weak motions that also moves along the light bridge. The dynamic short-lived jets above the LB seem to be guided by the magnetic field lines. Reconnection events are a likely trigger for such phenomenon since they occur at locations where the magnetic field changes orientation sharply. We find no clear relation between the jets and the photospheric flow pattern.

Accepted for publication in A&A, 9 pages, 7 figures

References in corpus (4)

• The Solar Optical Telescope for the Hinode Mission: An Overview
• CRISP Spectropolarimetric Imaging of Penumbral Fine Structure
• Detection of opposite polarities in a sunspot light bridge: evidence of low-altitude magnetic reconnection
• The GREGOR Fabry-Pérot Interferometer and its companion the Blue Imaging Solar Spectrometer

Cited by in corpus (20)

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• Chromospheric Plasma Ejections in a Light Bridge of a Sunspot
• A solar flare disturbing a light wall above a sunspot light bridge
• The formation of an atypical sunspot light bridge as a result of large-scale flux emergence
• Kinematics and Magnetic Properties of a Light Bridge in a Decaying Sunspot
• Sunspot Light Walls Suppressed by Nearby Brightenings
• Sunspot penumbral filaments intruding into a light bridge and the resultant reconnection jets
• Structure of sunspot light bridges in the chromosphere and transition region
• Long-Term Evolution of Three Light Bridges Developed on the Same Sunspot
• Fan-shaped jet close to a light bridge
• Small-scale Bright Blobs Ejected from a Sunspot Light Bridge
• Light Bridges Can Suppress the Formation of Coronal Loops
• Various Activities above Sunspot Light Bridges in IRIS Observations: Classification and Comparison
• Homologous flaring activity over a sunspot light bridge in an emerging active region
• Behaviour of oscillations in loop structures above active regions
• Investigation of a confined C-class flare in an arch filament system close to a regular sunspot