Articles | Volume 12, issue 3
Research article
15 Mar 2019
Research article |  | 15 Mar 2019

A new method of inferring the size, number density, and charge of mesospheric dust from its in situ collection by the DUSTY probe

Ove Havnes, Tarjei Antonsen, Gerd Baumgarten, Thomas W. Hartquist, Alexander Biebricher, Åshild Fredriksen, Martin Friedrich, and Jonas Hedin


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Ove Havnes on behalf of the Authors (11 Feb 2019)  Author's response
ED: Referee Nomination & Report Request started (12 Feb 2019) by Bernd Funke
RR by Anonymous Referee #1 (26 Feb 2019)
ED: Publish subject to technical corrections (27 Feb 2019) by Bernd Funke
Short summary
We present a new method of analyzing data from rocket-borne aerosol detectors of the Faraday cup type (DUSTY). By using models for how aerosols are charged in the mesosphere and how they interact in a collision with the probes, fundamental parameters like aerosol radius, charge, and number density can be derived. The resolution can be down to ~ 10 cm, which is much lower than other available methods. The theory is furthermore used to analyze DUSTY data from the 2016 rocket campaign MAXIDUSTY.