On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes

The dust probe DUSTY, first launched during the summer of 1994 (flights ECT–02 and ECT–07) from Andøya Rocket Range, northern Norway, was the first probe to unambiguously detect heavy charged mesospheric aerosols, from hereon referred to as dust. In ECT–02 the probe detected negatively charged dust...

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Published in:Annales Geophysicae
Main Authors: O. Havnes, L. I. Næsheim
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2007
Subjects:
Online Access:https://doi.org/10.5194/angeo-25-623-2007
https://doaj.org/article/4ee9678618634feaa7a7c78c78857aa6
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author O. Havnes
L. I. Næsheim
author_facet O. Havnes
L. I. Næsheim
author_sort O. Havnes
collection Directory of Open Access Journals: DOAJ Articles
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container_title Annales Geophysicae
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description The dust probe DUSTY, first launched during the summer of 1994 (flights ECT–02 and ECT–07) from Andøya Rocket Range, northern Norway, was the first probe to unambiguously detect heavy charged mesospheric aerosols, from hereon referred to as dust. In ECT–02 the probe detected negatively charged dust particles in the height interval of 83 to 88.5 km. In this flight, the lower grid in the detector (Grid 2) measures both positive and negative currents in various regions, and we find that the relationship between the current measurements of Grid 2 and the bottom plate can only be explained by influence from secondary charge production on Grid 2. In ECT–07, which had a large coning, positive currents reaching the top grid of the probe were interpreted as due to the impact of positively charged dust particles. We have now reanalyzed the data from ECT–07 and arrived at the conclusion that the measured positive currents to this grid must have been mainly due to secondary charging effects from the impacting dust particles. The grid consists of a set of parallel wires crossed with an identical set of wires on top of it, and we find that if the observed currents were created from the direct impact of charged dust particles, then they should be very weakly modulated at four times the rocket spin rate ω R . Observations show, however, that the observed currents are strongly modulated at 2ω R . We cannot reproduce the observed large modulations of the impact currents in the dust layer if the currents are due only to the transfer of the charges on the impacted dust particles. Based on the results of recent ice cluster impact secondary charging experiments by Tomsic (2003), which found that a small fraction of the ice clusters, when impacting with nearly grazing incidence, carried away one negative charge −1 e , we have arrived at the conclusion that similar, but significantly more effective, charging effects must be predominantly responsible for the positive currents measured by the top grid in ECT–07 and their large rotational ...
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spelling ftdoajarticles:oai:doaj.org/article:4ee9678618634feaa7a7c78c78857aa6 2025-01-16T18:56:18+00:00 On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes O. Havnes L. I. Næsheim 2007-03-01T00:00:00Z https://doi.org/10.5194/angeo-25-623-2007 https://doaj.org/article/4ee9678618634feaa7a7c78c78857aa6 EN eng Copernicus Publications https://www.ann-geophys.net/25/623/2007/angeo-25-623-2007.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-25-623-2007 0992-7689 1432-0576 https://doaj.org/article/4ee9678618634feaa7a7c78c78857aa6 Annales Geophysicae, Vol 25, Pp 623-637 (2007) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2007 ftdoajarticles https://doi.org/10.5194/angeo-25-623-2007 2022-12-30T22:49:51Z The dust probe DUSTY, first launched during the summer of 1994 (flights ECT–02 and ECT–07) from Andøya Rocket Range, northern Norway, was the first probe to unambiguously detect heavy charged mesospheric aerosols, from hereon referred to as dust. In ECT–02 the probe detected negatively charged dust particles in the height interval of 83 to 88.5 km. In this flight, the lower grid in the detector (Grid 2) measures both positive and negative currents in various regions, and we find that the relationship between the current measurements of Grid 2 and the bottom plate can only be explained by influence from secondary charge production on Grid 2. In ECT–07, which had a large coning, positive currents reaching the top grid of the probe were interpreted as due to the impact of positively charged dust particles. We have now reanalyzed the data from ECT–07 and arrived at the conclusion that the measured positive currents to this grid must have been mainly due to secondary charging effects from the impacting dust particles. The grid consists of a set of parallel wires crossed with an identical set of wires on top of it, and we find that if the observed currents were created from the direct impact of charged dust particles, then they should be very weakly modulated at four times the rocket spin rate ω R . Observations show, however, that the observed currents are strongly modulated at 2ω R . We cannot reproduce the observed large modulations of the impact currents in the dust layer if the currents are due only to the transfer of the charges on the impacted dust particles. Based on the results of recent ice cluster impact secondary charging experiments by Tomsic (2003), which found that a small fraction of the ice clusters, when impacting with nearly grazing incidence, carried away one negative charge −1 e , we have arrived at the conclusion that similar, but significantly more effective, charging effects must be predominantly responsible for the positive currents measured by the top grid in ECT–07 and their large rotational ... Article in Journal/Newspaper Andøya Northern Norway Directory of Open Access Journals: DOAJ Articles Andøya ENVELOPE(13.982,13.982,68.185,68.185) Norway Annales Geophysicae 25 3 623 637
spellingShingle Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
O. Havnes
L. I. Næsheim
On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title_full On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title_fullStr On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title_full_unstemmed On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title_short On the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
title_sort on the secondary charging effects and structure of mesospheric dust particles impacting on rocket probes
topic Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
topic_facet Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
url https://doi.org/10.5194/angeo-25-623-2007
https://doaj.org/article/4ee9678618634feaa7a7c78c78857aa6