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Tracing the Cosmic Energy Flow with Parker Solar Probe: Universal ProcessesHeliophysics is inherently interdisciplinary, born from multiple subjects to understand how the Sun interacts with its surrounding environment. Heliophysicists and Astrophysicists seldom exchange ideas since the scientific infrastructure partitions research areas by spatial location in the cosmos. Parker Solar Probe (PSP) is sending back puzzling information in regions we have never been before, presenting an opportunity to search for answers in non-traditional ways that are inherently cross-disciplinary. The fundamental processes that govern the physics of the universe, such as wave-particle interactions, turbulence, magnetic reconnection, and shocks, are mechanisms to study cosmic energy flow. We present PSP observations that may enable us to assess the universality of these fundamental processes in – and across boundaries of –various space and astrophysical regimes. Specifically, we focus on the exotic shapes of proton velocity distribution functions and subsequent evolution leading to multi-scale wave generation and particle acceleration. We welcome ideas, tools, and methodologies from all disciplines to understand the systems of systems governing our universe.
Document ID
20220015876
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
J L Verniero
(Goddard Space Flight Center Greenbelt, Maryland, United States)
T D Phan
(University of California, Berkeley Berkeley, California, United States)
A Brosius
(Pennsylvania State University State College, Pennsylvania, United States)
A Szabo
(Goddard Space Flight Center Greenbelt, Maryland, United States)
D E Larson
(University of California, Berkeley Berkeley, California, United States)
R Livi
(University of California, Berkeley Berkeley, California, United States)
P L Whittlesey
(University of California, Berkeley Berkeley, California, United States)
M D McManus
(University of California, Berkeley Berkeley, California, United States)
A Rahmati
(University of California, Berkeley Berkeley, California, United States)
O Romeo
(University of California, Berkeley Berkeley, California, United States)
K W Paulson
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
P S Pyakurel
(University of California, Berkeley Berkeley, California, United States)
T A Bowen
(University of California, Berkeley Berkeley, California, United States)
M Velli
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
O Panasenco
(Advanced Heliophysics Pasadena, California, United States)
J W Bonnell
(University of California, Berkeley Berkeley, California, United States)
B D G Chandran
(University of New Hampshire Durham, New Hampshire, United States)
S Badman
(Smithsonian Astrophysical Observatory Cambridge, Massachusetts, United States)
L B Wilson
(Goddard Space Flight Center Greenbelt, Maryland, United States)
J C Kasper
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
S D Bale
(University of California, Berkeley Berkeley, California, United States)
Date Acquired
October 21, 2022
Subject Category
Solar Physics
Meeting Information
Meeting: 20th Annual International Astrophysics Conference (AIAC)
Location: Santa Fe, NM
Country: US
Start Date: October 31, 2022
End Date: November 4, 2022
Sponsors: AIAC
Funding Number(s)
WBS: 388443.04.01
CONTRACT_GRANT: 80NSSC20M0189
CONTRACT_GRANT: NNN06AA01C
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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