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• W1744539053 abstract "[1] A recent survey of the Mars Global Surveyor (MGS) electron data for dayside photoelectron observations over regions of strong crustal fields revealed an unusual bimodal solar flux dependence. The elevated-flux population was associated with the timing of a large global dust storm in late 2001. The results of a systematic study parameterizing the photoelectron flux intensities against a solar flux proxy and MGS-observed atmospheric dust opacity are presented here. Instantaneous dust opacities were used as well as time-history averages and maximal values. The result is a functional form for the photoelectron fluxes against these parameters. The inclusion of instantaneous dust opacity values in the function do not improve the correlation, but a time-history window significantly enhances the correlation and explains the bimodal distribution in the electron fluxes. The best relationship was obtained with 7-Earth-month time-history dust opacity variables included in the function. The most likely explanation for this long-lived influence of dust storms is a composition and/or density change in the upper atmosphere." @default.
• W1744539053 created "2016-06-24" @default.
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• W1744539053 date "2012-06-01" @default.
• W1744539053 modified "2023-10-15" @default.
• W1744539053 title "Time‐history influence of global dust storms on the upper atmosphere at Mars" @default.
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• W1744539053 doi "https://doi.org/10.1029/2012gl051994" @default.
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