Genesis and Coronal-jet-generating Eruption of a Solar Minifilament Captured by IRIS Slit-raster Spectra
Navdeep K. Panesar, Sanjiv K. Tiwari, Ronald L. Moore, Alphonse C., Sterling, and Bart De Pontieu

TL;DR
This study captures the detailed spectral and imaging observations of a solar minifilament eruption that produces a coronal jet, revealing the magnetic and plasma dynamics involved in the process.
Contribution
First IRIS Mg II spectra fully capturing a minifilament eruption and jet formation, linking magnetic flux cancelation to jet initiation with detailed plasma diagnostics.
Findings
Minifilament forms above a flux cancelation neutral line.
Eruption involves blueshifted upflows and redshifted downflows.
IRIS spectra reveal plasma density, temperature, and Doppler speeds.
Abstract
We present the first IRIS Mg II slit-raster spectra that fully capture the genesis and coronal-jet-generating eruption of a central-disk solar minifilament. The minifilament arose in a negative-magnetic-polarity coronal hole. The Mg II spectroheliograms verify that the minifilament plasma temperature is chromospheric. The Mg II spectra show that the erupting minifilament's plasma has blueshifted upflow in the jet spire's onset and simultaneous redshifted downflow at the location of the compact jet bright point (JBP). From the Mg II spectra together with AIA EUV images and HMI magnetograms, we find: (i) the minifilament forms above a flux cancelation neutral line at an edge of a negative-polarity network flux clump; (ii) during the minifilament's fast-eruption onset and jet-spire onset, the JBP begins brightening over the flux-cancelation neutral line. From IRIS2 inversion of the Mg II…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
