activity
20082023
most citedObservation of multiple sausage oscillations in cool postflare loop

85 citations · 716 across the 21 of their papers we have counts for

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Showing astro-ph.SRShow all

13 papers · 1 filter

astro-ph.SR2023★ 31 cited

New Evidence on the Origin of Solar Wind Microstreams/Switchbacks

Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky +4

Microstreams are fluctuations in the solar wind speed and density associated with polarity-reversing folds in the magnetic field (also denoted switchbacks). Despite their long heri…

astro-ph.SR2022★ 32 cited

Plasmoids, Flows, and Jets During Magnetic Reconnection in a Failed Solar Eruption

Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos +3

We report a detailed analysis of a failed eruption and flare in active region 12018 on 2014 April 3 using multiwavelength observations from SDO/AIA, IRIS, STEREO, and Hinode/SOT. A…

astro-ph.SR2022★ 17 cited

Kink Oscillation of a Flux Rope During a Failed Solar Eruption

Pankaj Kumar, Valery M. Nakariakov, Judith T. Karpen +2

We report a decaying kink oscillation of a flux rope during a confined eruptive flare, observed off the solar limb by SDO/AIA, that lacked a detectable white-light coronal mass eje…

astro-ph.SR2022★ 57 cited

Quasiperiodic Energy Release and Jets at the Base of Solar Coronal Plumes

Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky +3

Coronal plumes are long, ray-like, open structures, which have been considered as possible sources for the solar wind. Their origin in the largely unipolar coronal holes has long b…

astro-ph.SR2020★ 46 cited

From Pseudostreamer Jets to CMEs: Observations of the Breakout Continuum

Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos +3

The magnetic breakout model, in which reconnection in the corona leads to destabilization of a filament channel, explains numerous features of eruptive solar events, from small-sca…

astro-ph.SR2019★ 60 cited

First Detection of Plasmoids from Breakout Reconnection on the Sun

Pankaj Kumar, Judith T. Karpen, Spiro K. Antiochos +2

Transient collimated plasma ejections (jets) occur frequently throughout the solar corona, in active regions, quiet Sun, and coronal holes. Although magnetic reconnection is genera…