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- W3105220960 abstract "We present a long-duration (∼10 yr) statistical analysis of the temperatures, plasma betas, and temperature ratios for the electron, proton, and alpha-particle populations observed by the Wind spacecraft near 1 au. The mean(median) scalar temperatures are Te,tot = 12.2(11.9) eV, Tp,tot = 12.7(8.6) eV, and Tα,tot = 23.9(10.8) eV. The mean(median) total plasma betas are βe,tot = 2.31(1.09), βp,tot = 1.79(1.05), and βα,tot = 0.17(0.05). The mean(median) temperature ratios are (Te/Tp)tot = 1.64(1.27), (Te/Tα)tot = 1.24(0.82), and (Tα/Tp)tot = 2.50(1.94). We also examined these parameters during time intervals that exclude interplanetary (IP) shocks, times within the magnetic obstacles (MOs) of interplanetary coronal mass ejections (ICMEs), and times that exclude MOs. The only times that show significant alterations to any of the parameters examined are those during MOs. In fact, the only parameter that does not show a significant change during MOs is the electron temperature. Although each parameter shows a broad range of values, the vast majority are near the median. We also compute particle–particle collision rates and compare to effective wave–particle collision rates. We find that, for reasonable assumptions of wave amplitude and occurrence rates, the effect of wave–particle interactions on the plasma is equal to or greater than the effect of Coulomb collisions. Thus, wave–particle interactions should not be neglected when modeling the solar wind." @default.
- W3105220960 created "2020-11-23" @default.
- W3105220960 creator A5000627540 @default.
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- W3105220960 creator A5050201056 @default.
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- W3105220960 creator A5091328515 @default.
- W3105220960 date "2018-06-01" @default.
- W3105220960 modified "2023-10-16" @default.
- W3105220960 title "The Statistical Properties of Solar Wind Temperature Parameters Near 1 au" @default.
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