activity
20172025
most citedA case-study of multi-temperature coronal jets for emerging flux MHD models

43 citations · 420 across the 34 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.SR2024

Magnetic Reconnection between a Solar Jet and a Filament Channel

Garima Karki, Brigitte Schmieder, Pooja Devi +4

The solar corona is highly structured by bunches of magnetic field lines forming either loops, or twisted flux ropes representing prominences/filaments, or very dynamic structures…

astro-ph.SR2024

High-resolution observational analysis of flare ribbon fine structures

Jonas Thoen Faber, Reetika Joshi, Luc Rouppe van der Voort +4

Context. Since the mechanism of energy release from solar flares is still not fully understood, the study of fine-scale features developing during flares becomes important for prog…

astro-ph.SR2024★ 11 cited

Study of the excitation of large amplitude oscillations in a prominence by nearby flares

Manuel Luna, Reetika Joshi, Brigitte Schmieder +3

Large amplitude oscillations commonly occur in solar prominences, triggered by energetic phenomena such as jets and flares. On March 14-15, 2015, a filament partially erupted in tw…

astro-ph.SR2024★ 18 cited

High-resolution observations of recurrent jets from an arch filament system

Reetika Joshi, Luc Rouppe van der Voort, Brigitte Schmieder +4

Solar jets are collimated plasma ejections along magnetic field lines observed in hot (EUV jets) and cool (chromospheric surges) temperature diagnostics. Their trigger mechanisms a…

astro-ph.SR2024★ 13 cited

Generic low-atmosphere signatures of swirled-anemone jets

Reetika Joshi, Guillaume Aulanier, Alice Radcliffe +4

Solar jets are collimated plasma flows moving along magnetic field lines and accelerated at low altitude following magnetic reconnection. Several of them originate from anemone-sha…