Vis enkel innførsel

dc.contributor.authorHavnes, Ove
dc.contributor.authorAntonsen, Tarjei
dc.contributor.authorBaumgarten, Gerd
dc.contributor.authorHartquist, Thomas W.
dc.contributor.authorBiebricher, Alexander
dc.contributor.authorFredriksen, Åshild
dc.contributor.authorFriedrich, Martin
dc.contributor.authorHedin, Jonas
dc.date.accessioned2019-10-16T12:55:21Z
dc.date.available2019-10-16T12:55:21Z
dc.date.issued2019-03-15
dc.description.abstract<p>We present a new method of analyzing measurements of mesospheric dust made with DUSTY rocket-borne Faraday cup probes. It can yield the variation in fundamental dust parameters through a mesospheric cloud with an altitude resolution down to 10 cm or less if plasma probes give the plasma density variations with similar height resolution. A DUSTY probe was the first probe that unambiguously detected charged dust and aerosol particles in the Earth's mesosphere. DUSTY excluded the ambient plasma by various biased grids, which however allowed dust particles with radii above a few nanometers to enter, and it measured the flux of charged dust particles. The flux measurements directly yielded the total ambient dust charge density. <p>We extend the analysis of DUSTY data by using the impact currents on its main grid and the bottom plate as before, together with a dust charging model and a secondary charge production model, to allow the determination of fundamental parameters, such as dust radius, charge number, and total dust density. We demonstrate the utility of the new analysis technique by considering observations made with the DUSTY probes during the MAXIDUSTY rocket campaign in June–July 2016 and comparing the results with those of other instruments (lidar and photometer) also used in the campaign. In the present version we have used monodisperse dust size distributions.en_US
dc.descriptionSource at <a href=https://doi.org/10.5194/amt-12-1673-2019>https://doi.org/10.5194/amt-12-1673-2019</a>.en_US
dc.identifier.citationHavnes, O., Antonsen, T., Baumgarten, G., Hartquist, T.W., Biebricher, A., Fredriksen, Å., Friedrich, M. & Hedin, J. (2019). A new method of inferring the size, number density, and charge of mesospheric dust from its in situ collection by the DUSTY probe. <i>Atmospheric Measurement Techniques, 12</i>(3), 1673-1683. https://doi.org/10.5194/amt-12-1673-2019en_US
dc.identifier.cristinIDFRIDAID 1686343
dc.identifier.doi10.5194/amt-12-1673-2019
dc.identifier.issn1867-8548
dc.identifier.urihttps://hdl.handle.net/10037/16418
dc.language.isoengen_US
dc.publisherEuropean Geosciences Unionen_US
dc.relation.isbasedonHavnes, O., Antonsen, T., Baumgarten, G., Hartquist, T., Biebricher, A., Fredriksen, Å., Friedrich, M. & Hedin, J. (2018). Replication Data for: A new method to inference the size, number density, and charge of mesospheric dust from its in situ collection by the DUSTY probe. <a href=https://doi.org/10.18710/LEMXBU>https://doi.org/10.18710/LEMXBU</a>. DataverseNO, V1, UNF:6:Y7zgKZilxKVVzRrC2f3Hrg== [fileUNF]en_US
dc.relation.journalAtmospheric Measurement Techniques
dc.relation.projectIDinfo:eu-repo/grantAgreement/RCN/ROMFORSK/240065/Norway/In Situ,Remote,and Laboratory Investigations of Mesospheric Aerosols/Dust and Their Role in Atmospheric Chemical and Physical Processes//en_US
dc.rights.accessRightsopenAccessen_US
dc.subjectVDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438en_US
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk, astronomi: 438en_US
dc.titleA new method of inferring the size, number density, and charge of mesospheric dust from its in situ collection by the DUSTY probeen_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US
dc.typePeer revieweden_US


Tilhørende fil(er)

Thumbnail

Denne innførselen finnes i følgende samling(er)

Vis enkel innførsel