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A Living Catalog of Stream Interaction Regions in the Parker Solar Probe EraStream interaction regions (SIRs) and corotating interaction regions (CIRs) are important phenomena in heliospheric physics. These large-scale structures vary temporally and spatially, both in latitude and with radial distance. The additions of Parker Solar Probe(PSP) and Solar Orbiter have allowed for investigations into the radial evolution of these structures over a wide range of heliocentric distances for the first time since the Helios era. To better enable investigations of SIRs and CIRs within the inner heliosphere, we have developed a living catalog of SIR and CIR observations by Parker Solar Probe with corresponding observations by STEREO-A as well as ACE and Wind at 1 au. The methodology used for the identification of events and the generation of this catalog, the initial catalog of PSP observations spanning orbits one through five along with corresponding 1 au observations, and information on accessing the living catalog for future studies is described. This list of SIR and CIR events from PSP and corresponding observations from other heliophysics missions will enable case studies utilizing unique orbital arrangements, as well as aid in future statistical studies to further understand the properties and evolution of these structures.
Document ID
20210026629
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
R. C. Allen
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
G C Ho
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
L. K. Jian
(Goddard Space Flight Center Greenbelt, Maryland, United States)
S. K. Vines
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
S. D. Bale
(University of California, Berkeley Berkeley, California, United States)
A. W. Case
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
M. E. Hill
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
C. J. Joyce
(Princeton University Princeton, New Jersey, United States)
J. C. Kasper
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
K. E. Korreck
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
D. M. Malaspina
(University of Colorado Boulder Boulder, Colorado, United States)
D. J. McComas
(Princeton University Princeton, New Jersey, United States)
R. McNutt
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
C. Möstl
(Space Research Institute Graz, Austria)
D. Odstrcil
(Goddard Space Flight Center Greenbelt, Maryland, United States)
N Raouafi
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
N A Schwadron
(University of New Hampshire Durham, New Hampshire, United States)
M. L. Stevens
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
Date Acquired
January 11, 2022
Publication Date
June 2, 2021
Publication Information
Publication: Astronomy & Astrophysics Special Issue
Publisher: EDP Sciences,
Volume: 650
Issue: A25
Issue Publication Date: June 2, 2021
ISSN: 0004-6361
e-ISSN: 1432-0746
Subject Category
Solar Physics
Funding Number(s)
WBS: 791926.02.03.06.64
CONTRACT_GRANT: NNN06AA01C
CONTRACT_GRANT: NNX17AC05G
CONTRACT_GRANT: HQ-NASA-HPAC
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
Catalogs
Solar wind
Acceleration of particles
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