Coulomb collisional analysis of solar wind ions

Author(s)Johnson, Elliot T.
Date Accessioned2024-10-29T16:43:04Z
Date Available2024-10-29T16:43:04Z
Publication Date2024
SWORD Update2024-10-13T22:02:12Z
AbstractOwing to its low density and high temperature, the solar wind frequently exhibits strong departures from local thermodynamic equilibrium (LTE). Previous studies have focused on non-LTE features but were largely limited to using observations from single spacecrafts. In contrast, this research utilized contemporaneous, in-situ observations from two different spacecraft at two different distances from the Sun. Collisional analysis combines the effects of collisional relaxation and large-scale expansion, quantifying how ion relative temperature and differential flow evolve through the heliosphere. This generates a prediction for the distribution of these quantities in the solar wind at any distance from the Sun. Results suggest that ion relative temperature and differential flow through the inner heliosphere is largely governed by the effects of expansion and Coulomb collisions, and that preferential heating is largely limited to the corona.
AdvisorMaruca, Bennett A.
DegreePh.D.
DepartmentUniversity of Delaware, Department of Physics and Astronomy
DOIhttps://doi.org/10.58088/k748-ts24
Unique Identifier1504406809
URLhttps://udspace.udel.edu/handle/19716/35475
Languageen
PublisherUniversity of Delaware
URIhttps://www.proquest.com/pqdtlocal1006271/dissertations-theses/coulomb-collisional-analysis-solar-wind-ions/docview/3116496553/sem-2?accountid=10457
KeywordsCollision physics
KeywordsCoulomb collisions
KeywordsPlasma
KeywordsSolar wind
KeywordsSun
TitleCoulomb collisional analysis of solar wind ions
TypeThesis
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