Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31763
Titolo: | Acceleration of Solar Energetic Particles through CME-driven Shock and Streamer Interaction | Autori: | FRASSATI, FEDERICA LAURENZA, MONICA BEMPORAD, Alessandro West, Matthew J. MANCUSO, Salvatore SUSINO, ROBERTO ALBERTI, TOMMASO ROMANO, Paolo |
Data pubblicazione: | 2022 | Rivista: | THE ASTROPHYSICAL JOURNAL | Numero: | 926 | Fascicolo: | 2 | Da pagina:: | 227 | Abstract: | On 2013 June 21, a solar prominence eruption was observed, accompanied by an M2.9 class flare, a fast coronal mass ejection, and a type II radio burst. The concomitant emission of solar energetic particles (SEPs) produced a significant proton flux increase, in the energy range 4-100 MeV, measured by the Low and High Energy Telescopes on board the Solar TErrestrial RElations Observatory (STEREO)-B spacecraft. Only small enhancements, at lower energies, were observed at the STEREO-A and Geostationary Operational Environmental Satellite (GOES) spacecraft. This work investigates the relationship between the expanding front, coronal streamers, and the SEP fluxes observed at different locations. Extreme-ultraviolet data, acquired by the Atmospheric Imaging Assembly (AIA) instrument on board the Solar Dynamics Observatory (SDO), were used to study the expanding front and its interaction with streamer structures in the low corona. The 3D shape of the expanding front was reconstructed and extrapolated at different times by using SDO/AIA, STEREO/Sun Earth Connection Coronal and Heliospheric Investigation, and Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph observations with a spheroidal model. By adopting a potential field source surface approximation and estimating the magnetic connection of the Parker spiral, below and above 2.5 R ⊙, we found that during the early expansion of the eruption, the front had a strong magnetic connection with STEREO-B (between the nose and flank of the eruption front) while having a weak connection with STEREO-A and GOES. The obtained results provide evidence, for the first time, that the interaction between an expanding front and streamer structures can be responsible for the acceleration of high-energy SEPs up to at least 100 MeV, as it favors particle trapping and hence increases the shock acceleration efficiency. | URI: | http://hdl.handle.net/20.500.12386/31763 | URL: | https://iopscience.iop.org/article/10.3847/1538-4357/ac460e | ISSN: | 0004-637X | DOI: | 10.3847/1538-4357/ac460e | Bibcode ADS: | 2022ApJ...926..227F | Fulltext: | open |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
Frassati_2022_ApJ_926_227_compressed.pdf | Pdf editoriale | 9.75 MB | Adobe PDF | Visualizza/apri |
Page view(s)
102
controllato il 11-set-2024
Download(s)
25
controllato il 11-set-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.