A Laboratory Experiment of Magnetic Reconnection: Outflows, Heating and Waves in Chromospheric Jets
N. Nishizuka, Y. Hayashi, H. Tanabe, A. Kuwahata, Y. Kaminou, Y. Ono,, M. Inomoto, T. Shimizu

TL;DR
This laboratory experiment simulates chromospheric magnetic reconnection, revealing plasma outflows, heating, and wave phenomena, thus providing insights into the physics of solar chromospheric jets.
Contribution
The study experimentally reproduces key features of chromospheric jets through component reconnection, bridging the gap between solar observations and laboratory plasma physics.
Findings
Bi-directional plasma outflows up to 5 km/s observed
Ion heating exceeding 30 eV in downstream regions
Magnetic fluctuations with periods of 5-10 microseconds
Abstract
Hinode observations have revealed intermittent recurrent plasma ejections/jets in the chromosphere. These are interpreted as a result of non-perfectly anti-parallel magnetic reconnection, i.e. component reconnection, between a twisted magnetic flux tube and the pre-existing coronal/chromospheric magnetic field, though the fundamental physics of component reconnection is unrevealed. In this paper, we experimentally reproduced the magnetic configuration and investigated the dynamics of plasma ejections, heating and wave generation triggered by component reconnection in the chromosphere. We set plasma parameters as in the chromosphere (density 10^14 cm^-3, temperature 5-10 eV, i.e. (5-10)x10^4 K, and reconnection magnetic field 200 G) using argon plasma. Our experiment shows bi-directional outflows with the speed of 5 km/s at maximum, ion heating in the downstream area over 30 eV and…
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