Journal articles
Observations of Heating along Intermittent Structures in the Inner Heliosphere from PSP Data
R.A. Qudsi
1
B. A. Maruca
2
W.H. Matthaeus
2
T. N. Parashar
1
Riddhi Bandyopadhyay
1
R. Chhiber
1, 2
A. Chasapis
3
Melvyn L. Goldstein
4
S.D. Bale
5, 6
J.W. Bonnell
5
Thierry Dudok de Wit
7
K. Goetz
8
P.R. Harvey
5
R.J Macdowall
4
D. Malaspina
3
Marc Pulupa
5
J.C. Kasper
9
K.E. Korreck
9
A.W. Case
9
M. Stevens
9
P. Whittlesey
5
D. Larson
5
R. Livi
10
M. Velli
11
N. Raouafi
12
Riddhi Bandyopadhyay 1
Author
R. Chhiber 1, 2
Author
A. Chasapis 3
Author
Melvyn L. Goldstein 4
Author
S.D. Bale 5, 6
Author
J.W. Bonnell 5
Author
Thierry Dudok de Wit 7
Author IdHAL : thierry-dudok-de-wit ORCID : https://orcid.org/0000-0002-4401-0943
K. Goetz 8
Author
N. Raouafi 12
Author
1
University of Delaware [Newark] (Newark, DE 19716 USA - United States)
2
Bartol Research Institute (Department of Physics and Astronomy, University of Delaware, Newak, 19716 Delaware - United States)
- University of Delaware [Newark] (Newark, DE 19716 USA - United States)
3
LASP - Laboratory for Atmospheric and Space Physics [Boulder] (1234 Innovation Drive, Boulder, CO 80303-7814 - United States)
- University of Colorado [Boulder] (Boulder, Colorado 80309 - United States)
4
GSFC - NASA Goddard Space Flight Center (Greenbelt, MD 20771 - United States)
5
University of California [Berkeley] (Berkeley, CA - United States)
- University of California (United States)
6
Imperial College London (South Kensington Campus, London SW7 2AZ - United Kingdom)
7
LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (3A, Avenue de la Recherche Scientifique 45071 Orléans cedex 2 - France)
- OSUC - Observatoire des Sciences de l'Univers en région Centre : UMS3116 (Campus Géosciences, 1A rue de la Férollerie, 45071 Orléans - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UO - Université d'Orléans (Château de la Source - Avenue du Parc Floral - BP 6749 - 45067 Orléans cedex 2 - France)
- CNRS - Centre National de la Recherche Scientifique : UMS3116 (France)
- CNES - Centre National d’Études Spatiales [Paris] : UMR 7328 (Siège social : 2 place Maurice Quentin, 75039 Paris - France)
8
University of Minnesota [Twin Cities] (Minneapolis/St.Paul - United States)
- University of Minnesota System (United States)
9
Smithsonian Astrophysical Observatory (60 Garden Street, MS 67, Cambridge, MA 02138-1516 - United States)
- Smithsonian Institution (PO Box 37012, Washington, DC 20013-7012 - United States)
10
SSL - Space Sciences Laboratory [Berkeley] (7 Gauss Way, Berkeley, CA 94720 - United States)
- University of California [Berkeley] (Berkeley, CA - United States)
- University of California (United States)
11
EPSS - Department of Earth, Planetary and Space Sciences [Los Angeles] (Los Angeles, CA 90095-1567 - United States)
- UCLA - University of California [Los Angeles] ( Los Angeles, Californie 90095 - United States)
- University of California (United States)
12
APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (11100 Johns Hopkins Road, Laurel, Maryland - United States)
Abstract : The solar wind proton temperature at 1 au has been found to be correlated with small-scale intermittent magnetic structures, i.e., regions with enhanced temperature are associated with coherent structures, such as current sheets. Using Parker Solar Probe data from the first encounter, we study this association using measurements of the radial proton temperature, employing the partial variance of increments (PVI) technique to identify intermittent magnetic structures. We observe that the probability density functions of high PVI events have higher median temperatures than those with lower PVI. The regions in space where PVI peaks were also locations that had enhanced temperatures when compared with similar regions, suggesting a heating mechanism in the young solar wind that is associated with intermittency developed by a nonlinear turbulent cascade in the immediate vicinity.
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Journal articles
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https://hal-insu.archives-ouvertes.fr/insu-02942198
Contributor : Nathalie Pothier <>
Submitted on : Friday, September 18, 2020 - 7:43:06 AM
Last modification on : Wednesday, September 23, 2020 - 4:36:29 AM
Long-term archiving on: : Friday, December 4, 2020 - 5:06:26 PM
Contributor : Nathalie Pothier <>
Submitted on : Friday, September 18, 2020 - 7:43:06 AM
Last modification on : Wednesday, September 23, 2020 - 4:36:29 AM
Long-term archiving on: : Friday, December 4, 2020 - 5:06:26 PM
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Identifiers
- HAL Id : insu-02942198, version 1
- DOI : 10.3847/1538-4365/ab5c19
Citation
R.A. Qudsi, B. A. Maruca, W.H. Matthaeus, T. N. Parashar, Riddhi Bandyopadhyay, et al.. Observations of Heating along Intermittent Structures in the Inner Heliosphere from PSP Data. Astrophysical Journal Supplement, American Astronomical Society, 2020, 246 (2), pp.46. ⟨10.3847/1538-4365/ab5c19⟩. ⟨insu-02942198⟩
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