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Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions
DOI: 10.1007/s11207-024-02373-0 Bibcode: 2024SoPh..299..129G

Firoz, K. A.; Grechnev, V. V.; Lysenko, A. L. +3 more

The SOL2012-05-17 event is remarkable in that it caused one of two ground-level enhancements (GLE71) in Solar Cycle 24. Despite the efforts spent studying this solar event, some aspects of it remain unclear. This relates to the development of a coronal mass ejection (CME), the history of the shock wave, and the flare. Our measurements reveal the f…

2024 Solar Physics
PROBA-2 SOHO 2
On the Instrumental Discrepancies in Lyman-Alpha Observations of Solar Flares
DOI: 10.1007/s11207-024-02407-7 Bibcode: 2024SoPh..299..162G

Dammasch, Ingolf E.; Milligan, Ryan O.; Greatorex, Harry J.

Despite the energetic significance of Lyman-alpha (Lyα; 1216 Å) emission from solar flares, regular observations of flare related Lyα have been relatively scarce until recently. Advances …

2024 Solar Physics
PROBA-2 0
Probing Velocity Dispersion Inside Coronal Mass Ejections: New Insights on Their Initiation
DOI: 10.3847/2041-8213/ad5da5 Bibcode: 2024ApJ...970L..17M

Mierla, Marilena; Reiss, Martin A.; Banerjee, Dipankar +4 more

This work studies the kinematics of the leading edge and the core of six coronal mass ejections (CMEs) in the combined field of view of Sun Watcher using Active Pixel System detector and Image Processing (SWAP) on board PRoject for On-Board Autonomy (PROBA-2) and the ground-based K-Cor coronagraph of the Mauna Loa Solar Observatory. We report, for…

2024 The Astrophysical Journal
PROBA-2 SOHO 0
Localization of the Gamma-Ray Emission Region in the 1 September 2014 Behind-the-Limb Solar Flare According to the Fermi/LAT Data
DOI: 10.1007/s11207-024-02264-4 Bibcode: 2024SoPh..299...18K

Grechnev, V. V.; Kochanov, A. A.; Kiselev, V. I. +1 more

Since the launch of the Fermi mission in 2008, it has become possible to study high-energy solar γ-rays with an unprecedented imaging capability. In particular, the position of the >100 MeVγ-ray source can shed light on the origin of high-energy protons that is still controversial. However, the imaging of solar γ-ray sources with the Fermi Larg…

2024 Solar Physics
PROBA-2 0