Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays

Tietueen suppeat tiedot
dc.contributor.authorAguilar M.
dc.contributor.authorCavasonza L.A.
dc.contributor.authorAmbrosi G.
dc.contributor.authorArruda L.
dc.contributor.authorAttig N.
dc.contributor.authorBagwell C.
dc.contributor.authorBarao F.
dc.contributor.authorBarrin L.
dc.contributor.authorBartoloni A.
dc.contributor.authorBaşeǧmez-Du Pree S.
dc.contributor.authorBattiston R.
dc.contributor.authorBehlmann M.
dc.contributor.authorBelyaev N.
dc.contributor.authorBerdugo J.
dc.contributor.authorBertucci B.
dc.contributor.authorBindi V.
dc.contributor.authorBollweg K.
dc.contributor.authorBolster J.
dc.contributor.authorBorgia B.
dc.contributor.authorBoschini M.J.
dc.contributor.authorBourquin M.
dc.contributor.authorBueno E.F.
dc.contributor.authorBurger J.
dc.contributor.authorBurger W.J.
dc.contributor.authorBurmeister S.
dc.contributor.authorCai X.D.
dc.contributor.authorCapell M.
dc.contributor.authorCasaus J.
dc.contributor.authorCastellini G.
dc.contributor.authorCervelli F.
dc.contributor.authorChang Y.H.
dc.contributor.authorChen G.M.
dc.contributor.authorChen G.R.
dc.contributor.authorChen H.S.
dc.contributor.authorChen Y.
dc.contributor.authorCheng L.
dc.contributor.authorChou H.Y.
dc.contributor.authorChouridou S.
dc.contributor.authorChoutko V.
dc.contributor.authorChung C.H.
dc.contributor.authorClark C.
dc.contributor.authorCoignet G.
dc.contributor.authorConsolandi C.
dc.contributor.authorContin A.
dc.contributor.authorCorti C.
dc.contributor.authorCui Z.
dc.contributor.authorDadzie K.
dc.contributor.authorDass A.
dc.contributor.authorDelgado C.
dc.contributor.authorDella Torre S.
dc.contributor.authorDemirköz M.B.
dc.contributor.authorDerome L.
dc.contributor.authorDi Falco S.
dc.contributor.authorDi Felice V.
dc.contributor.authorDíaz C.
dc.contributor.authorDimiccoli F.
dc.contributor.authorVon Doetinchem P.
dc.contributor.authorDong F.
dc.contributor.authorDonnini F.
dc.contributor.authorDuranti M.
dc.contributor.authorEgorov A.
dc.contributor.authorEline A.
dc.contributor.authorFaldi F.
dc.contributor.authorFeng J.
dc.contributor.authorFiandrini E.
dc.contributor.authorFisher P.
dc.contributor.authorFormato V.
dc.contributor.authorFreeman C.
dc.contributor.authorGámez C.
dc.contributor.authorGarcía-López R.J.
dc.contributor.authorGargiulo C.
dc.contributor.authorGast H.
dc.contributor.authorGervasi M.
dc.contributor.authorGiovacchini F.
dc.contributor.authorGómez-Coral D.M.
dc.contributor.authorGong J.
dc.contributor.authorGoy C.
dc.contributor.authorGrabski V.
dc.contributor.authorGrandi D.
dc.contributor.authorGraziani M.
dc.contributor.authorGuracho A.N.
dc.contributor.authorHaino S.
dc.contributor.authorHan K.C.
dc.contributor.authorHashmani R.K.
dc.contributor.authorHe Z.H.
dc.contributor.authorHeber B.
dc.contributor.authorHsieh T.H.
dc.contributor.authorHu J.Y.
dc.contributor.authorIncagli M.
dc.contributor.authorJang W.Y.
dc.contributor.authorJia Y.
dc.contributor.authorJinchi H.
dc.contributor.authorKaragöz G.
dc.contributor.authorKhiali B.
dc.contributor.authorKim G.N.
dc.contributor.authorKirn T.
dc.contributor.authorKounina O.
dc.contributor.authorKounine A.
dc.contributor.authorKoutsenko V.
dc.contributor.authorKrasnopevtsev D.
dc.contributor.authorKuhlman A.
dc.contributor.authorKulemzin A.
dc.contributor.authorLa Vacca G.
dc.contributor.authorLaudi E.
dc.contributor.authorLaurenti G.
dc.contributor.authorLavecchia G.
dc.contributor.authorLazzizzera I.
dc.contributor.authorLee H.T.
dc.contributor.authorLee S.C.
dc.contributor.authorLi H.L.
dc.contributor.authorLi J.Q.
dc.contributor.authorLi M.
dc.contributor.authorLi Q.
dc.contributor.authorLi Q.Y.
dc.contributor.authorLi S.
dc.contributor.authorLi S.L.
dc.contributor.authorLi J.H.
dc.contributor.authorLi Z.H.
dc.contributor.authorLiang J.
dc.contributor.authorLiang M.J.
dc.contributor.authorLight C.
dc.contributor.authorLin C.H.
dc.contributor.authorLippert T.
dc.contributor.authorLiu J.H.
dc.contributor.authorLu S.Q.
dc.contributor.authorLu Y.S.
dc.contributor.authorLuebelsmeyer K.
dc.contributor.authorLuo J.Z.
dc.contributor.authorLuo X.
dc.contributor.authorMacHate F.
dc.contributor.authorMañá C.
dc.contributor.authorMarín J.
dc.contributor.authorMarquardt J.
dc.contributor.authorMartin T.
dc.contributor.authorMartínez G.
dc.contributor.authorMasi N.
dc.contributor.authorMaurin D.
dc.contributor.authorMedvedeva T.
dc.contributor.authorMenchaca-Rocha A.
dc.contributor.authorMeng Q.
dc.contributor.authorMikhailov V.V.
dc.contributor.authorMolero M.
dc.contributor.authorMott P.
dc.contributor.authorMussolin L.
dc.contributor.authorNegrete J.
dc.contributor.authorNikonov N.
dc.contributor.authorNozzoli F.
dc.contributor.authorOcampo-Peleteiro J.
dc.contributor.authorOliva A.
dc.contributor.authorOrcinha M.
dc.contributor.authorPalermo M.
dc.contributor.authorPalmonari F.
dc.contributor.authorPaniccia M.
dc.contributor.authorPashnin A.
dc.contributor.authorPauluzzi M.
dc.contributor.authorPensotti S.
dc.contributor.authorPlyaskin V.
dc.contributor.authorPohl M.
dc.contributor.authorPoluianov S.
dc.contributor.authorQin X.
dc.contributor.authorQu Z.Y.
dc.contributor.authorQuadrani L.
dc.contributor.authorRancoita P.G.
dc.contributor.authorRapin D.
dc.contributor.authorConde A.R.
dc.contributor.authorRobyn E.
dc.contributor.authorRosier-Lees S.
dc.contributor.authorRozhkov A.
dc.contributor.authorRozza D.
dc.contributor.authorSagdeev R.
dc.contributor.authorSchael S.
dc.contributor.authorVon Dratzig A.S.
dc.contributor.authorSchwering G.
dc.contributor.authorSeo E.S.
dc.contributor.authorShan B.S.
dc.contributor.authorSiedenburg T.
dc.contributor.authorSong J.W.
dc.contributor.authorSong X.J.
dc.contributor.authorSonnabend R.
dc.contributor.authorStrigari L.
dc.contributor.authorSu T.
dc.contributor.authorSun Q.
dc.contributor.authorSun Z.T.
dc.contributor.authorTacconi M.
dc.contributor.authorTang X.W.
dc.contributor.authorTang Z.C.
dc.contributor.authorTian J.
dc.contributor.authorTing S.C.C.
dc.contributor.authorTing S.M.
dc.contributor.authorTomassetti N.
dc.contributor.authorTorsti J.
dc.contributor.authorUrban T.
dc.contributor.authorUsoskin I.
dc.contributor.authorVagelli V.
dc.contributor.authorVainio R.
dc.contributor.authorValencia-Otero M.
dc.contributor.authorValente E.
dc.contributor.authorValtonen E.
dc.contributor.authorVázquez Acosta M.
dc.contributor.authorVecchi M.
dc.contributor.authorVelasco M.
dc.contributor.authorVialle J.P.
dc.contributor.authorWang C.X.
dc.contributor.authorWang L.
dc.contributor.authorWang L.Q.
dc.contributor.authorWang N.H.
dc.contributor.authorWang Q.L.
dc.contributor.authorWang S.
dc.contributor.authorWang X.
dc.contributor.authorWang Y.
dc.contributor.authorWang Z.M.
dc.contributor.authorWei J.
dc.contributor.authorWeng Z.L.
dc.contributor.authorWu H.
dc.contributor.authorXiong R.Q.
dc.contributor.authorXu W.
dc.contributor.authorYan Q.
dc.contributor.authorYang Y.
dc.contributor.authorYashin I.I.
dc.contributor.authorYelland A.
dc.contributor.authorYi H.
dc.contributor.authorYu Y.M.
dc.contributor.authorYu Z.Q.
dc.contributor.authorZannoni M.
dc.contributor.authorZhang C.
dc.contributor.authorZhang F.
dc.contributor.authorZhang F.Z.
dc.contributor.authorZhang J.H.
dc.contributor.authorZhang Z.
dc.contributor.authorZhao F.
dc.contributor.authorZheng C.
dc.contributor.authorZheng Z.M.
dc.contributor.authorZhuang H.L.
dc.contributor.authorZhukov V.
dc.contributor.authorZichichi A.
dc.contributor.authorZuccon P.
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.contributor.organization-code2606702
dc.converis.publication-id179577235
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/179577235
dc.date.accessioned2025-08-27T21:52:37Z
dc.date.available2025-08-27T21:52:37Z
dc.description.abstract<p>We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0 × 10<sup>8</sup> electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6σ at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.</p>
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid201318
dc.identifier.oldhandle10024/184345
dc.identifier.urihttps://www.utupub.fi/handle/11111/47996
dc.identifier.urlhttps://doi.org/10.1103/PhysRevLett.130.161001
dc.identifier.urnURN:NBN:fi-fe2023052547816
dc.language.isoen
dc.okm.affiliatedauthorTorsti, Jarmo
dc.okm.affiliatedauthorVainio, Rami
dc.okm.affiliatedauthorValtonen, Eino
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.typeA1 ScientificArticle
dc.publisherAmerican Physical Society
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumber161001
dc.relation.doi10.1103/PhysRevLett.130.161001
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue16
dc.relation.volume130
dc.source.identifierhttps://www.utupub.fi/handle/10024/184345
dc.titleTemporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays
dc.year.issued2023

Tiedostot

Näytetään 1 - 1 / 1
Name:
TorstiEtAl2023TemporalStructuresInElectronSpectra.pdf
Size:
4.68 MB
Format:
Adobe Portable Document Format
Lataa

Kokoelmat

Rinnakkaistallenteet