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dc.contributor.authorChristian, E.R.
dc.contributor.authorCohen, C.M.S.
dc.contributor.authorCummings, A.C.
dc.contributor.authorDavis, A.J.
dc.contributor.authorDesai, M.I.
dc.contributor.authorde Nolfo, G.A.
dc.contributor.authorGiacalone, J.
dc.contributor.authorHill, M.E.
dc.contributor.authorJoyce, C.J.
dc.contributor.authorLabrador, A.W.
dc.contributor.authorLeske, R.A.
dc.contributor.authorMatthaeus, W.H.
dc.contributor.authorMcComas, D.J.
dc.contributor.authorMcNutt, R.L., Jr.
dc.contributor.authorMewaldt, R.A.
dc.contributor.authorMitchell, D.G.
dc.contributor.authorMitchell, J.G.
dc.contributor.authorRankin, J.S.
dc.contributor.authorRoelof, E.C.
dc.contributor.authorSchwadron, N.A.
dc.contributor.authorStone, E.C.
dc.contributor.authorSzalay, J.R.
dc.contributor.authorWiedenbeck, M.E.
dc.date.accessioned2023-12-22T05:07:00Z
dc.date.available2023-12-22T05:07:00Z
dc.date.issued2022-03-18
dc.identifier.citationChristian, E., Cohen, C., Cummings, A. C., Davis, A., Desai, M., De Nolfo, G. A., ... & Wiedenbeck, M. (2022, March). New Data from the ISʘIS instrument Suite on Parker Solar Probe. In 37th International Cosmic Ray Conference. 12-23 July 2021. Berlin (p. 1306).
dc.identifier.issn1824-8039
dc.identifier.doi10.22323/1.395.1306
dc.identifier.urihttp://hdl.handle.net/10150/670595
dc.description.abstractNASA's Parker Solar Probe (PSP) mission's first seven orbits include perihelia as close as ~11 million km (~16 solar radii), much closer to the Sun than any prior human-made object. Onboard PSP, the Integrated Science Investigation of the Sun (IS☉IS) instrument suite makes groundbreaking measurements of solar energetic particles (SEPs). Here we discuss the near-Sun energetic particle radiation environment over PSP's first two and a half years, which reveal where and how energetic particles are energized and transported. We find a great variety of energetic particle events accelerated both locally and remotely. These include stream and co-rotating interaction regions (SIRs and CIRs), “impulsive” SEP events driven by magnetic reconnection near the Sun, and events related to Coronal Mass Ejections (CMEs). These IS☉IS observations made close to the Sun provide critical information for investigating the near-Sun transport and energization of solar energetic particles, which has been difficult to resolve from prior observations. The Parker Solar Probe IS☉IS data are made public soon after receipt at Earth (which can be many months after the observations). We will also discuss how to get access to the data. © Copyright owned by the author(s) under the terms of the Creative Commons.
dc.language.isoen
dc.publisherSissa Medialab Srl
dc.rights© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.titleNew Data from the IS☉IS Instrument Suite on Parker Solar Probe
dc.typeProceedings
dc.typetext
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizona
dc.identifier.journalProceedings of Science
dc.description.noteOpen access journal
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleProceedings of Science
refterms.dateFOA2023-12-22T05:07:00Z


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© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
Except where otherwise noted, this item's license is described as © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).