Abstract

Abstract. MASS (Mesospheric Aerosol Sampling Spectrometer) is a multichannel mass spectrometer for charged aerosol particles, which was flown from the Andøya Rocket Range, Norway, through NLC and PMSE on 3 August 2007 and through PMSE on 6 August 2007. The eight-channel analyzers provided for the first time simultaneous measurements of the charge density residing on aerosol particles in four mass ranges, corresponding to ice particles with radii <0.5 nm (including ions), 0.5–1 nm, 1–2 nm, and >3 nm (approximately). Positive and negative particles were recorded on separate channels. Faraday rotation measurements provided electron density and a means of checking charge density measurements made by the spectrometer. Additional complementary measurements were made by rocket-borne dust impact detectors, electric field booms, a photometer and ground-based radar and lidar. The MASS data from the first flight showed negative charge number densities of 1500–3000 cm−3 for particles with radii >3 nm from 83–88 km approximately coincident with PMSE observed by the ALWIN radar and NLC observed by the ALOMAR lidar. For particles in the 1–2 nm range, number densities of positive and negative charge were similar in magnitude (~2000 cm−3) and for smaller particles, 0.5–1 nm in radius, positive charge was dominant. The occurrence of positive charge on the aerosol particles of the smallest size and predominately negative charge on the particles of largest size suggests that nucleation occurs on positive condensation nuclei and is followed by collection of negative charge during subsequent growth to larger size. Faraday rotation measurements show a bite-out in electron density that increases the time for positive aerosol particles to be neutralized and charged negatively. The larger particles (>3 nm) are observed throughout the NLC region, 83–88 km, and the smaller particles are observed primarily at the high end of the range, 86–88 km. The second flight into PMSE alone at 84–88 km, found only small number densities (~500 cm−3) of particles >3 nm in a narrow altitude range, 86.5–87.5 km. Both positive (~2000 cm−3) and negative (~4500 cm−3) particles with radii 1–2 nm were detected from 85–87.5 km.

Highlights

  • The noctilucent clouds (NLC) that appear in the polar summer mesosphere result from the growth of ice on condensation nuclei that may be meteoritic dust particles or ions (Turco et al, 1982; Hunten et al, 1980; Witt, 1969)

  • The number density of the charged fraction of the aerosol particles has been deduced from the data of these charge-collecting instruments and is of order 103 cm−3, which is much greater than the number densities of visible NLC particles

  • We present data from two flights of rocket-borne multichannel mass analyzers for charged aerosol particles that were flown into Polar Mesosphere Summer Echoes (PMSE) and NLC on 3 August 2007 (MASS1) and into PMSE alone on 6 August 2007 (MASS2)

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Summary

Introduction

The noctilucent clouds (NLC) that appear in the polar summer mesosphere result from the growth of ice on condensation nuclei that may be meteoritic dust particles or ions (Turco et al, 1982; Hunten et al, 1980; Witt, 1969). Much less is known about the subvisual aerosol particles, these have a significantly larger number density The detection of these particles by rocket-borne instruments is made possible through the collection of the charge they carry. Havnes et al (1996) flew a Faraday cup through NLC and found negative particles and positive particles in number densities too large to be accounted for by the standard plasma charging model. The number density of the charged fraction of the aerosol particles has been deduced from the data of these charge-collecting instruments and is of order 103 cm−3, which is much greater than the number densities of visible NLC particles. The data show that within the NLC/PMSE region at 83–88 km on 3 August 2007, particles with radii >3 nm were predominately negative with charge number densities up to 3000 cm−3.

The MASS payloads
MASS1 flight data
Launch conditions for MASS1
Launch conditions
Electron density
Channels 1–4
Quasineutrality check for MASS1 and MASS2
Positive ions
Positive charge on the smallest particles
Photometer data and the altitude dependence of particle size
Findings
Comparison with SOFIE limb scans
Summary and conclusion
Full Text
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