activity
20172026
most citedThe European Solar Telescope

99 citations · 618 across the 36 of their papers we have counts for

collaborators
Showing 2024Show all

8 papers · 1 filter

astro-ph.SR2024★ 5 cited

Three-part structure of solar coronal mass ejection observed in low coronal signatures of Solar Orbiter

Tatiana Podladchikova, Shantanu Jain, Astrid M. Veronig +4

This study examines the relationship between early solar coronal mass ejection (CME) propagation, the associated filament eruption, and coronal dimming in the rare event observed o…

astro-ph.SR2024

Estimating early coronal mass ejection propagation direction with DIRECD during the severe May 8 and follow-up June 8, 2024 events

Shantanu Jain, Tatiana Podladchikova, Astrid M. Veronig +4

On May 8, 2024, solar active region 13664 produced an X-class flare, several M-class flares, and multiple Earth-directed Coronal Mass Ejections (CMEs). The initial CME caused coron…

astro-ph.SR2024

Recovery of coronal dimmings

Giulia M. Ronca, Galina Chikunova, Karin Dissauer +2

Coronal dimmings are regions of reduced emission in the lower corona, observed after coronal mass ejections (CMEs) and representing their footprints. In order to investigate the lo…

astro-ph.SR2024

Multipoint study of the rapid filament evolution during a confined C2 flare on 28 March 2022, leading to eruption

Stefan Purkhart, Astrid M. Veronig, Bernhard Kliem +5

We studied the rapid filament evolution in AR 12975 during a confined C2 flare on 28 March 2022, which led to an eruptive M4 flare 1.5 h later. It is characterized by the breakup o…

astro-ph.SR2024★ 28 cited

A Universal Method for Solar Filament Detection from H-alpha Observations using Semi-supervised Deep Learning

Andrea Diercke, Robert Jarolim, Christoph Kuckein +7

Filaments are omnipresent features in the solar atmosphere. Their location, properties and time evolution can provide information about changes in solar activity and assist the ope…

astro-ph.SR2024

The McNish and Lincoln Solar Activity Predictions: The Method and its Performance

Frédéric Clette, Shantanu Jain, Tatiana Podladchikova

The McNish and Lincoln (ML) method, introduced in 1949, was one of the first attempts to produce mid-term forecasts of solar activity, up to 12 months ahead. However, it has been p…