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• W2897350560 startingPage "1706" @default.
• W2897350560 abstract "Robustly identifying the solar sources of individual packets of solar wind measured in interplanetary space remains an open problem. We set out to see if this problem is easier to tackle using solar wind measurements closer to the Sun than 1 AU, where the mixing and dynamical interaction of different solar wind streams is reduced. Using measurements from the Helios mission, we examined how the proton core temperature anisotropy and cross helicity varied with distance. At 0.3 AU there are two clearly separated anisotropic and isotropic populations of solar wind, that are not distinguishable at 1 AU. The anisotropic population is always Alfv'enic and spans a wide range of speeds. In contrast the isotropic population has slow speeds, and contains a mix of Alfv'enic wind with constant mass fluxes, and non-Alfv'enic wind with large and highly varying mass fluxes. We split the in-situ measurements into three categories according these observations, and suggest that these categories correspond to wind that originated in the core of coronal holes, in or near active regions or the edges of coronal holes, and as small transients form streamers or pseudostreamers. Although our method by itself is simplistic, it provides a new tool that can be used in combination with other methods for identifying the sources of solar wind measured by Parker Solar Probe and Solar Orbiter." @default.
• W2897350560 created "2018-10-26" @default.
• W2897350560 creator A5012637868 @default.
• W2897350560 creator A5041800777 @default.
• W2897350560 creator A5044041585 @default.
• W2897350560 date "2018-10-22" @default.
• W2897350560 modified "2023-10-15" @default.
• W2897350560 title "Diagnosing solar wind origins using<i>in situ</i>measurements in the inner heliosphere" @default.
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• W2897350560 doi "https://doi.org/10.1093/mnras/sty2814" @default.
• W2897350560 hasPublicationYear "2018" @default.
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