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20132026
most citedFast magnetic reconnection in the solar chromosphere mediated by the plasmoid instability

145 citations · 753 across the 26 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.SR2018★ 42 cited

Subarcsecond blobs in flare-related coronal jets

Q. M. Zhang, L. Ni

In this paper, we report our multiwavelength observations of subarcsecond blobs in coronal jets. In AR 12149, a C5.5 circular-ribbon flare occurred on 2014 August 24. Two jets (jet…

astro-ph.SR2018★ 38 cited

Onset of secondary instabilities and plasma heating during magnetic reconnection in strongly magnetized regions of the low solar atmosphere

Lei Ni, Vyacheslav S. Lukin

We numerically study magnetic reconnection on different spatial scales and at different heights in the weakly ionized plasma of the low solar atmosphere (around ~km above…

astro-ph.SR2018★ 25 cited

Magnetic reconnection in the low solar chromosphere with a more realistic radiative cooling model

Lei Ni, Vyacheslav S. Lukin, Nicholas A. Murphy +1

Magnetic reconnection is the most likely mechanism responsible for the high temperature events that are observed in strongly magnetized locations around the temperature minimum in…

astro-ph.SR2018★ 18 cited

Numerical Studies of the Kelvin-Hemholtz Instability in the Coronal Jet

Tianle Zhao, Lei Ni, Jun Lin +1

The Kelvin-Hemholtz (K-H) instability in the corona EUV jet is studied via 2.5 MHD numerical simulations. The jet results from magnetic reconnection due to the interation of the ne…

astro-ph.SR2018★ 94 cited

Frequently Occurring Reconnection Jets from Sunspot Light Bridges

Hui Tian, Vasyl Yurchyshyn, Hardi Peter +12

Solid evidence of magnetic reconnection is rarely reported within sunspots, the darkest regions with the strongest magnetic fields and lowest temperatures in the solar atmosphere.…