The first ground-level enhancement of solar cycle 25 on 28 October 2021

dc.contributor.authorPapaioannou A
dc.contributor.authorKouloumvakos A
dc.contributor.authorMishev A
dc.contributor.authorVainio R
dc.contributor.authorUsoskin I
dc.contributor.authorHerbst K
dc.contributor.authorRouillard AP
dc.contributor.authorAnastasiadis A
dc.contributor.authorGieseler J
dc.contributor.authorWimmer-Schweingruber R
dc.contributor.authorKuhl P
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id175186089
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/175186089
dc.date.accessioned2022-10-28T12:25:56Z
dc.date.available2022-10-28T12:25:56Z
dc.description.abstract<p>Aims. The first relativistic solar proton event of solar cycle 25 was detected on 28 October 2021 by neutron monitors (NMs) on the ground and particle detectors on board spacecraft in near-Earth space. This is the first ground-level enhancement (GLE) of the current cycle. A detailed reconstruction of the NM response together with the identification of the solar eruption that generated these particles is investigated based on in situ and remote-sensing measurements. <br></p><p>Methods. In situ proton observations from a few MeV to similar to 500 MeV were combined with the detection of a solar flare in soft X-rays, a coronal mass ejection, radio bursts, and extreme ultraviolet (EUV) observations to identify the solar origin of the GLE. Timing analysis was performed, and a relation to the solar sources was outlined. <br></p><p>Results. GLE73 reached a maximum particle rigidity of similar to 2.4 GV and is associated with type III, type II, and type IV radio bursts and an EUV wave. A diversity of time profiles recorded by NMs was observed. This points to the event having an anisotropic nature. The peak flux at E & x2004;>& x2004;10 MeV was only similar to 30 pfu and remained at this level for several days. The release time of >= 1 GV particles was found to be similar to 15:40 UT. GLE73 had a moderately hard rigidity spectrum at very high energies (gamma & x2004;similar to & x2004;5.5). Comparison of GLE73 to previous GLEs with similar solar drivers is performed.</p>
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid176342
dc.identifier.oldhandle10024/159436
dc.identifier.urihttps://www.utupub.fi/handle/11111/31729
dc.identifier.urlhttps://www.aanda.org/articles/aa/full_html/2022/04/aa42855-21/aa42855-21.html
dc.identifier.urnURN:NBN:fi-fe2022081154026
dc.language.isoen
dc.okm.affiliatedauthorVainio, Rami
dc.okm.affiliatedauthorGieseler, Jan
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeB1 Scientific Journal
dc.publisherEDP SCIENCES S A
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberL5
dc.relation.doi10.1051/0004-6361/202142855
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume660
dc.source.identifierhttps://www.utupub.fi/handle/10024/159436
dc.titleThe first ground-level enhancement of solar cycle 25 on 28 October 2021
dc.year.issued2022

Tiedostot

Näytetään 1 - 1 / 1
Ladataan...
Name:
2202.07927.pdf
Size:
3.82 MB
Format:
Adobe Portable Document Format