262 citations · 7.1k across the 165 of their papers we have counts for
165 papers
Multi-point study of the energy release and transport in the 28 March 2022, M4-flare using STIX, EUI, and AIA during the first Solar Orbiter nominal mission perihelion
Stefan Purkhart, Astrid M. Veronig, Ewan C. M. Dickson +6
We present a case study of an M4-class flare on 28 March 2022, near Solar Orbiter's first science perihelion (0.33 AU). Solar Orbiter was 83.5° west of the Sun-Earth line, making t…
Onset and evolution of solar flares: Application of 2D and 3D models of magnetic reconnection
Bhuwan Joshi, Prabir K. Mitra, Astrid M. Veronig +1
The contemporary multi-wavelength observations have revealed various important features during solar flares which, on one hand, support the two-dimensional (2D) "standard flare mod…
On the three-dimensional relation between the coronal dimming, erupting filament and CME. Case study of the 28 October 2021 X1.0 event
Galina Chikunova, Tatiana Podladchikova, Karin Dissauer +4
We investigate the relation between the spatiotemporal evolution of the dimming region and the dominant direction of the filament eruption and CME propagation for the 28 October 20…
CME Propagation Through the Heliosphere: Status and Future of Observations and Model Development
M. Temmer, C. Scolini, I. G. Richardson +31
The ISWAT clusters H1+H2 have a focus on interplanetary space and its characteristics, especially on the large-scale co-rotating and transient structures impacting Earth. SIRs, gen…
Complete replacement of magnetic flux in a flux rope during a coronal mass ejection
Tingyu Gou, Rui Liu, Astrid M. Veronig +5
Solar coronal mass ejections are the most energetic events in the Solar System. In their standard formation model, a magnetic flux rope builds up into a coronal mass ejection throu…
Exploring magnetic field properties at the boundary of solar pores: A comparative study based on SDO-HMI observations
J. I. Campos Rozo, S. Vargas Domínguez, D. Utz +2
The Sun's magnetic fields play an important role in various solar phenomena. Solar pores are regions of intensified magnetic field strength compared to the surrounding photospheric…