J/ApJS/263/22ivo://CDS.VizieR/J/ApJS/263/22doi:10.26093/cds/vizier.22630022CDSHart S.T.Dayeh M.A.Bucik R.Desai M.I.Ebert R.W.Ho G.C.Li G.,Mason G.M.2023-10-16T12:09:05Z2023-04-11T17:07:10ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frthe-sunchemical-abundancesUsing ion measurements from Ultra-Low-Energy Isotope Spectrometer observations on board Advanced Composition Explorer and Solar Isotope Spectrometer observations on board the Solar Terrestrial Observatory (STEREO)-A and STEREO-B spacecraft, we have identified 854 ^3^He-rich time periods between 1997 September and 2021 March. We include all event types with observed ^3^He enhancements such as corotating interaction regions, gradual solar energetic particle (SEP) events, interplanetary shocks, and impulsive SEP events. We employ two different mass separation techniques to obtain ^3^He, ^4^He, Fe, and O fluences for each event, and we determine the ^3^He/^4^He and Fe/O abundance ratios between 0.32-0.45 and 0.64-1.28MeV/nucleon. We find a clear correlation in the ^3^He/^4^He and Fe/O abundance ratios between both energy ranges. We find two distinct trends in the ^3^He/^4^He versus Fe/O relation. For low ^3^He/^4^He values, there is a positive linear correlation between ^3^He/^4^He and Fe/O. However, at ^3^He/^4^He~0.3, Fe/O appears to reach a limit and the correlation weakens significantly. We provide a live catalog of ^3^He-rich time periods that includes the robust determination of the onset and end times of the 3He enhancements in SEP-associated periods for different types of events observed by multiple spacecraft. This catalog is available for public use. New releases will follow after major additions such as adding new periods from new missions (e.g., Parker Solar Probe and Solar Orbiter), identifying event types (impulsive SEP events, etc.), or adding new parameters such as remote observations detailing characteristics of the events' active regions.2022ApJS..263...22Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/263/22CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/AZh/75/586 : Abundances in solar atmosphere (Boyarchuk+, 1998)J/A+A/347/348 : Solar abundance of iron (Grevesse+, 1999)J/A+A/508/1403 : Oxygen lines in solar granulation. II. (Pereira+, 2009)J/ApJ/871/93 : Solar wind speed from ACE spacecraft 5yr data (Wang+, 2019)J/ApJ/893/78 : Streamer wave events from STEREO obs. (Decraemer+, 2020)J/ApJ/900/123 : Abundances of heavy ions in ICMEs from 1998-2011 (Gu+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/263/22https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/263/22http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/263/22https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/263/22https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/263/22http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/263/22GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/263/22/table1^3^He-rich time periods live catalog (1st edition)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEvent[1/854] Event numbermeta.id;meta.mainintStartStart time; YYYY/MM/DDThh:mm:ssstime.epochnullableStopStop time; YYYY/MM/DDThh:mm:ssstime.epochnullableStart-DOY[1/366] Start day of the yeartime.startdoubleStop-DOY[1.8/369] Stop day of the yeartime.endfloatTelMission identifier (1)meta.id;instr.telcharHe3/He4-1[0.01/43.8]? The ^3^He/^4^He abundance ratio (2)phys.abund.Y;arith.ratiodoublenullablee_He3/He4-1[0.0006/26.5]? Uncertainty in He3He4-1 (2)stat.errordoublenullableHe3/He4-2[0.009/52.6]? The ^3^He/^4^He^4^ abundance ratio (3)phys.abund.Y;arith.ratiodoublenullablee_He3/He4-2[0.0009/198]? Uncertainty in He3He4-2 (3)stat.errordoublenullableFe/O-1[0.01/6.5]? The Fe/O abundance ratio (2)phys.abunddoublenullablee_Fe/O-1[0.005/5.5]? Uncertainty in Fe/O-1 (2)stat.error;phys.abund.FedoublenullableFe/O-2[0.01/10.5]? The Fe/O abundance ratio (3)phys.abunddoublenullablee_Fe/O-2[0.006/9.5]? Uncertainty in Fe/O-2 (3)stat.error;phys.abund.Fedoublenullable