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- W3043016898 abstract "<p>The Parker Solar Probe (PSP) mission has completed 4 encounters through the solar corona significantly closer to the Sun than previous measurements. While PSP does not have a dedicated dust detector, measurements by the various instruments can provide insights into the dust environment in the inner heliosphere. &#160;Throughout the PSP orbit, interplanetary dust is impacting the spacecraft.&#160; Three-dimensional reconstructions of FIELDS observations show that the rate and direction of the dust impacts varies throughout the PSP orbit.&#160; During the encounter WISPR also finds the rate of impacts changes through the encounter period, but also a decrease in the intensity of the light scattered by the dust particles.&#160; The smooth decrease in the WISPR intensity beginning at about 0.1 AU is consistent with the production of Beta-meteroids seen by FIELDS. In this presentation, we will discuss the observations from the FIELDS and WISPR instruments and discuss initial models of the dust environment.&#160; The authors acknowledge support from the NASA Parker Solar Probe program.</p>" @default.
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- W3043016898 date "2020-03-23" @default.
- W3043016898 modified "2023-09-25" @default.
- W3043016898 title "The Dust Environment in the Inner Heliosphere" @default.
- W3043016898 doi "https://doi.org/10.5194/egusphere-egu2020-19398" @default.
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