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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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ANGEO | Articles | Volume 38, issue 4
Ann. Geophys., 38, 919–930, 2020
https://doi.org/10.5194/angeo-38-919-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 38, 919–930, 2020
https://doi.org/10.5194/angeo-38-919-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 03 Aug 2020

Regular paper | 03 Aug 2020

Dust sputtering within the inner heliosphere: a modelling study

Carsten Baumann et al.

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Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to minor revisions (review by editor) (23 Jun 2020) by Johan De Keyser
AR by Carsten Baumann on behalf of the Authors (23 Jun 2020)  Author's response    Manuscript
ED: Publish as is (30 Jun 2020) by Johan De Keyser
Publications Copernicus
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Short summary
Dust grains exist throughout our solar system. This dust is subject to destruction processes like sublimation and sputtering. Sputtering is the erosion of dust through the impact solar wind and can be very effective near the Sun. We performed calculations to find out how important the sputtering process is compared to the sublimation of dust. Recently launched spacecraft will probe the proximity of the Sun and measure the dust population. Our work will help to understand these measurements.
Dust grains exist throughout our solar system. This dust is subject to destruction processes...
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