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- W4251897427 abstract "It is now well-established through multiple event and statistical studies that the solar wind at 1 AU contains contains periodic, mesoscale (L~100-1000Mm) structures in the proton density. Composition variations observed within these structures and remote sensing observations of similar structures in the young solar wind indicate that at least some of these periodic structures originate in the solar atmosphere as a part of solar wind formation. Viall et al. [2008] analyzed 11 years of data from the Wind spacecraft near L1 and demonstrated a recurrence to the observed length scales of periodic structures in the solar wind proton density. In the time since that study, Wind has collected 14 additional years of solar wind data, new moment analysis of the Wind SWE data is available, and new methods for spectral background approximation have been developed. In this study, we analyze 25 years of Wind data collected near L1 and produce occurrence distributions of statistically significant periodic length scales in proton density. The results significantly expand upon the Viall et al. [2008] study, and further shows a possible relation of the length scales to solar “termination” events." @default.
- W4251897427 created "2022-05-12" @default.
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- W4251897427 date "2020-04-02" @default.
- W4251897427 modified "2023-10-16" @default.
- W4251897427 title "Inherent length scales of periodic mesoscale density structures in the solar wind over two solar cycles" @default.
- W4251897427 doi "https://doi.org/10.1002/essoar.10502592.1" @default.
- W4251897427 hasPublicationYear "2020" @default.
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