Energetic Particle Increases Associated with Stream Interaction Regions
The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the Energetic Particle Instrument-Hi (EPI-Hi, one of the two energetic particle instruments comprising the Integrated Science Investigation of t...
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| Veröffentlicht in: | The Astrophysical journal. Supplement series 2020-02, Vol.246 (2), p.20 |
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| creator | Cohen, C. M. S. Christian, E. R. Cummings, A. C. Davis, A. J. Desai, M. I. Giacalone, J. Hill, M. E. Joyce, C. J. Labrador, A. W. Leske, R. A. Matthaeus, W. H. McComas, D. J. McNutt, R. L. Mewaldt, R. A. Mitchell, D. G. Rankin, J. S. Roelof, E. C. Schwadron, N. A. Stone, E. C. Szalay, J. R. Wiedenbeck, M. E. Allen, R. C. Ho, G. C. Jian, L. K. Lario, D. Odstrcil, D. Bale, S. D. Badman, S. T. Pulupa, M. MacDowall, R. J. Kasper, J. C. Case, A. W. Korreck, K. E. Larson, D. E. Livi, Roberto Stevens, M. L. Whittlesey, Phyllis |
| description | The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the Energetic Particle Instrument-Hi (EPI-Hi, one of the two energetic particle instruments comprising the Integrated Science Investigation of the Sun, IS IS) measured seven proton intensity increases associated with stream interaction regions (SIRs), two of which appear to be occurring in the same region corotating with the Sun. The events are relatively weak, with observed proton spectra extending to only a few MeV and lasting for a few days. The proton spectra are best characterized by power laws with indices ranging from −4.3 to −6.5, generally softer than events associated with SIRs observed at 1 au and beyond. Helium spectra were also obtained with similar indices, allowing He/H abundance ratios to be calculated for each event. We find values of 0.016-0.031, which are consistent with ratios obtained previously for corotating interaction region events with fast solar wind ≤600 km s−1. Using the observed solar wind data combined with solar wind simulations, we study the solar wind structures associated with these events and identify additional spacecraft near 1 au appropriately positioned to observe the same structures after some corotation. Examination of the energetic particle observations from these spacecraft yields two events that may correspond to the energetic particle increases seen by EPI-Hi earlier. |
| doi_str_mv | 10.3847/1538-4365/ab4c38 |
| format | Article |
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M. S. ; Christian, E. R. ; Cummings, A. C. ; Davis, A. J. ; Desai, M. I. ; Giacalone, J. ; Hill, M. E. ; Joyce, C. J. ; Labrador, A. W. ; Leske, R. A. ; Matthaeus, W. H. ; McComas, D. J. ; McNutt, R. L. ; Mewaldt, R. A. ; Mitchell, D. G. ; Rankin, J. S. ; Roelof, E. C. ; Schwadron, N. A. ; Stone, E. C. ; Szalay, J. R. ; Wiedenbeck, M. E. ; Allen, R. C. ; Ho, G. C. ; Jian, L. K. ; Lario, D. ; Odstrcil, D. ; Bale, S. D. ; Badman, S. T. ; Pulupa, M. ; MacDowall, R. J. ; Kasper, J. C. ; Case, A. W. ; Korreck, K. E. ; Larson, D. E. ; Livi, Roberto ; Stevens, M. L. ; Whittlesey, Phyllis</creator><creatorcontrib>Cohen, C. M. S. ; Christian, E. R. ; Cummings, A. C. ; Davis, A. J. ; Desai, M. I. ; Giacalone, J. ; Hill, M. E. ; Joyce, C. J. ; Labrador, A. W. ; Leske, R. A. ; Matthaeus, W. H. ; McComas, D. J. ; McNutt, R. L. ; Mewaldt, R. A. ; Mitchell, D. G. ; Rankin, J. S. ; Roelof, E. C. ; Schwadron, N. A. ; Stone, E. C. ; Szalay, J. R. ; Wiedenbeck, M. E. ; Allen, R. C. ; Ho, G. C. ; Jian, L. K. ; Lario, D. ; Odstrcil, D. ; Bale, S. D. ; Badman, S. T. ; Pulupa, M. ; MacDowall, R. J. ; Kasper, J. C. ; Case, A. W. ; Korreck, K. E. ; Larson, D. E. ; Livi, Roberto ; Stevens, M. L. ; Whittlesey, Phyllis</creatorcontrib><description>The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the Energetic Particle Instrument-Hi (EPI-Hi, one of the two energetic particle instruments comprising the Integrated Science Investigation of the Sun, IS IS) measured seven proton intensity increases associated with stream interaction regions (SIRs), two of which appear to be occurring in the same region corotating with the Sun. The events are relatively weak, with observed proton spectra extending to only a few MeV and lasting for a few days. The proton spectra are best characterized by power laws with indices ranging from −4.3 to −6.5, generally softer than events associated with SIRs observed at 1 au and beyond. Helium spectra were also obtained with similar indices, allowing He/H abundance ratios to be calculated for each event. We find values of 0.016-0.031, which are consistent with ratios obtained previously for corotating interaction region events with fast solar wind ≤600 km s−1. Using the observed solar wind data combined with solar wind simulations, we study the solar wind structures associated with these events and identify additional spacecraft near 1 au appropriately positioned to observe the same structures after some corotation. Examination of the energetic particle observations from these spacecraft yields two events that may correspond to the energetic particle increases seen by EPI-Hi earlier.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.3847/1538-4365/ab4c38</identifier><language>eng</language><publisher>Saskatoon: The American Astronomical Society</publisher><subject>Corotating Interaction Regions (CIR) ; Corotation ; Energetic particles ; Fast solar wind ; Helium ; Perihelions ; Protons ; Solar activity ; Solar energetic particles ; Solar probes ; Solar wind ; Solar wind structure ; Spacecraft ; Spectra</subject><ispartof>The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.20</ispartof><rights>2020. The American Astronomical Society. 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M. S.</creatorcontrib><creatorcontrib>Christian, E. R.</creatorcontrib><creatorcontrib>Cummings, A. C.</creatorcontrib><creatorcontrib>Davis, A. J.</creatorcontrib><creatorcontrib>Desai, M. I.</creatorcontrib><creatorcontrib>Giacalone, J.</creatorcontrib><creatorcontrib>Hill, M. E.</creatorcontrib><creatorcontrib>Joyce, C. J.</creatorcontrib><creatorcontrib>Labrador, A. W.</creatorcontrib><creatorcontrib>Leske, R. A.</creatorcontrib><creatorcontrib>Matthaeus, W. H.</creatorcontrib><creatorcontrib>McComas, D. J.</creatorcontrib><creatorcontrib>McNutt, R. L.</creatorcontrib><creatorcontrib>Mewaldt, R. A.</creatorcontrib><creatorcontrib>Mitchell, D. G.</creatorcontrib><creatorcontrib>Rankin, J. S.</creatorcontrib><creatorcontrib>Roelof, E. C.</creatorcontrib><creatorcontrib>Schwadron, N. A.</creatorcontrib><creatorcontrib>Stone, E. C.</creatorcontrib><creatorcontrib>Szalay, J. R.</creatorcontrib><creatorcontrib>Wiedenbeck, M. E.</creatorcontrib><creatorcontrib>Allen, R. 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We find values of 0.016-0.031, which are consistent with ratios obtained previously for corotating interaction region events with fast solar wind ≤600 km s−1. Using the observed solar wind data combined with solar wind simulations, we study the solar wind structures associated with these events and identify additional spacecraft near 1 au appropriately positioned to observe the same structures after some corotation. 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L.</au><au>Whittlesey, Phyllis</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Energetic Particle Increases Associated with Stream Interaction Regions</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><stitle>APJS</stitle><addtitle>Astrophys. J. Suppl</addtitle><date>2020-02-01</date><risdate>2020</risdate><volume>246</volume><issue>2</issue><spage>20</spage><pages>20-</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the Energetic Particle Instrument-Hi (EPI-Hi, one of the two energetic particle instruments comprising the Integrated Science Investigation of the Sun, IS IS) measured seven proton intensity increases associated with stream interaction regions (SIRs), two of which appear to be occurring in the same region corotating with the Sun. The events are relatively weak, with observed proton spectra extending to only a few MeV and lasting for a few days. The proton spectra are best characterized by power laws with indices ranging from −4.3 to −6.5, generally softer than events associated with SIRs observed at 1 au and beyond. Helium spectra were also obtained with similar indices, allowing He/H abundance ratios to be calculated for each event. We find values of 0.016-0.031, which are consistent with ratios obtained previously for corotating interaction region events with fast solar wind ≤600 km s−1. Using the observed solar wind data combined with solar wind simulations, we study the solar wind structures associated with these events and identify additional spacecraft near 1 au appropriately positioned to observe the same structures after some corotation. Examination of the energetic particle observations from these spacecraft yields two events that may correspond to the energetic particle increases seen by EPI-Hi earlier.</abstract><cop>Saskatoon</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4365/ab4c38</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0003-3112-4201</orcidid><orcidid>https://orcid.org/0000-0002-8111-1444</orcidid><orcidid>https://orcid.org/0000-0003-1960-2119</orcidid><orcidid>https://orcid.org/0000-0003-2685-9801</orcidid><orcidid>https://orcid.org/0000-0002-6849-5527</orcidid><orcidid>https://orcid.org/0000-0002-7728-0085</orcidid><orcidid>https://orcid.org/0000-0002-1573-7457</orcidid><orcidid>https://orcid.org/0000-0001-7224-6024</orcidid><orcidid>https://orcid.org/0000-0002-5674-4936</orcidid><orcidid>https://orcid.org/0000-0002-3841-5020</orcidid><orcidid>https://orcid.org/0000-0002-7077-930X</orcidid><orcidid>https://orcid.org/0000-0002-1989-3596</orcidid><orcidid>https://orcid.org/0000-0002-3840-7696</orcidid><orcidid>https://orcid.org/0000-0002-3520-4041</orcidid><orcidid>https://orcid.org/0000-0003-2079-5683</orcidid><orcidid>https://orcid.org/0000-0003-2134-3937</orcidid><orcidid>https://orcid.org/0000-0002-3176-8704</orcidid><orcidid>https://orcid.org/0000-0001-6160-1158</orcidid><orcidid>https://orcid.org/0000-0002-7318-6008</orcidid><orcidid>https://orcid.org/0000-0002-0156-2414</orcidid><orcidid>https://orcid.org/0000-0002-6145-436X</orcidid><orcidid>https://orcid.org/0000-0001-6095-2490</orcidid><orcidid>https://orcid.org/0000-0002-3737-9283</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0067-0049 |
| ispartof | The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.20 |
| issn | 0067-0049 1538-4365 |
| language | eng |
| recordid | cdi_iop_journals_10_3847_1538_4365_ab4c38 |
| source | Institute of Physics Open Access Journal Titles |
| subjects | Corotating Interaction Regions (CIR) Corotation Energetic particles Fast solar wind Helium Perihelions Protons Solar activity Solar energetic particles Solar probes Solar wind Solar wind structure Spacecraft Spectra |
| title | Energetic Particle Increases Associated with Stream Interaction Regions |
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