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- W1617772455 abstract "The present characterization of the Venus ionosphere gives attention to features observed by the Pioneer Venus orbiter in situ ionospheric particle measuring instrument over an entire cycle of solar activity. A striking change is noted in the typical ionospheric morphology from solar maximum to minimum. The principal source of ionization in the dayside ionosphere during both solar maximum and minimum is solar EUV radiation, while that in the nightside is a downward flux of O(+) ions that originate in the dayside ionosphere and are transported across the nightside hemisphere by a supersonic ion wind. The dayside ionosphere contains fluxes of suprathermal electrons whose energy spectra are consistent with fluxes originating in EUV photo production." @default.
- W1617772455 created "2016-06-24" @default.
- W1617772455 creator A5068581572 @default.
- W1617772455 date "2013-03-18" @default.
- W1617772455 modified "2023-10-17" @default.
- W1617772455 title "The Venus Ionosphere from in Situ Measurements" @default.
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- W1617772455 doi "https://doi.org/10.1029/gm066p0237" @default.
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