Multiple Solar Jets from NOAA AR 12644
Reetika Joshi, Ramesh Chandra
TL;DR
This paper reports on high-resolution observations of twelve recurring solar jets from NOAA AR 12644, triggered by magnetic reconnection at a low coronal null-point, highlighting the dynamic magnetic activity in the region.
Contribution
It provides detailed multi-band observational evidence linking magnetic flux changes to jet eruptions, emphasizing the role of magnetic reconnection in jet formation.
Findings
Twelve recurring jets observed from NOAA AR 12644.
Jets triggered by magnetic reconnection at a low coronal null-point.
Magnetic flux emergence and cancellation observed at jet locations.
Abstract
We present here the observations of solar jets observed on April 04, 2017 from NOAA active region (AR) 12644 using high temporal and spatial resolution AIA instrument. We have observed around twelve recurring jets during the whole day. Magnetic flux emergence and cancellation have been observed at the jet location. The multi-band observations evidenced that these jets were triggered due to the magnetic reconnection at low coronal null-point.
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