Simulations of the collection of mesospheric dust particles with a rocket instrument
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Published:2024-06-28
Issue:12
Volume:17
Page:3843-3861
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ISSN:1867-8548
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Container-title:Atmospheric Measurement Techniques
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language:en
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Short-container-title:Atmos. Meas. Tech.
Author:
Pineau AdrienORCID, Trollvik Henriette, Greaker Herman, Olsen Sveinung, Eilertsen Yngve, Mann IngridORCID
Abstract
Abstract. We investigate the collection of dust particles in the mesosphere with the MESS (MEteoric Smoke Sampler) instrument that is designed to fly on a sounding rocket. We assume that the ice particles that form in the polar mesosphere between 80 and 85 km altitude in summer contain meteoric smoke particles; and these should be collected with MESS. The instrument consists of a collection device with an opening and closure mechanism, as well as an attached conic funnel which increases the sampling area in comparison to the collection area. Dust particles are collected either directly after passing through the instrument or indirectly after colliding with and fragmenting on the funnel wall. We calculate the dust and fragment trajectories in the detector to determine the collection efficiency for different particle sizes, rocket velocities, and heights, and we find the final velocities and the temperatures of the particles. The considered design has a sampling area of 62.78 mm diameter and a collection area of 20 mm diameter. For the conditions at the rocket launch site in Andøya, Norway, we estimate the collection of meteoric smoke particles contained in the ice particles to be ∼ 1012–1014 amu mm−2. The estimated temperatures suggest that the composition of these smoke particles is not affected by the collection. Our calculations also show that keeping the instrument open above 85 km altitude increases the amount of small smoke particles that are directly collected. The directly collected smoke particles are heated as they decelerate, which can affect their composition.
Funder
Norges Forskningsråd Universitetet i Tromsø National Nuclear Security Administration University of Rochester New York State Energy Research and Development Authority
Publisher
Copernicus GmbH
Reference45 articles.
1. Antonsen, T. and Havnes, O.: On the detection of mesospheric meteoric smoke particles embedded in noctilucent cloud particles with rocket-borne dust probes, Rev. Sci. Instrum., 86, 033305, https://doi.org/10.1063/1.4914394, 2015. a, b, c, d, e, f 2. Antonsen, T., Mann, I., Vaverka, J., Nouzak, L., and Fredriksen, Å.: A comparison of contact charging and impact ionization in low-velocity impacts: implications for dust detection in space, Ann. Geophys., 39, 533–548, https://doi.org/10.5194/angeo-39-533-2021, 2021. a, b 3. Baines, M., Williams, I., Asebiomo, A., and Agacy, R.: Resistance to the motion of a small sphere moving through a gas, Mon. Not. R. Astron. Soc., 130, 63–74, 1965. a 4. Bardeen, C., Toon, O., Jensen, E., Marsh, D., and Harvey, V.: Numerical simulations of the three-dimensional distribution of meteoric dust in the mesosphere and upper stratosphere, J. Geophys. Res.-Atmos., 113, D17202, https://doi.org/10.1029/2007JD009515, 2008. a, b, c 5. Baumann, C., Rapp, M., Kero, A., and Enell, C.-F.: Meteor smoke influences on the D-region charge balance – review of recent in situ measurements and one-dimensional model results, Ann. Geophys., 31, 2049–2062, https://doi.org/10.5194/angeo-31-2049-2013, 2013. a
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