Abstract

Abstract. We report measurements of dust currents obtained with a small probe and a larger probe during the flight of the ECOMA-4 rocket through the summer polar mesosphere. The payload included two small dust probes behind a larger dust probe located centrally at the front. For certain phases of the payload rotation, the current registered by one of the small dust probes was up to 2 times the current measured with the larger probe, even though the effective collection area of the larger probe was 4 times that of the small one. We analyze the phase dependence of the currents and their difference with a model based on the assumption that the small probe was hit by charged dust fragments produced in collisions of mesospheric dust with the payload body. Our results confirm earlier findings that secondary charge production in the collision of a noctilucent cloud/Polar Summer Mesospheric Echo (NLC/PMSE) dust particle with the payload body must be several orders of magnitude larger than might be expected from laboratory studies of collisions of pure ice particles with a variety of clean surfaces. An important consequence is that for some payload configurations, one should not assume that the current measured with a detector used to study mesospheric dust is simply proportional to the number density of ambient dust particles. The higher secondary charge production may be due to the NLC/PMSE particles containing multiple meteoric smoke particles.

Highlights

  • Polar Mesospheric Summer Echoes (PMSEs) are radar features formed near the mesopause (e.g. Rapp and Lubken, 2004)

  • We suggest that the largest magnitudes of the University of Tromsø (UiT) probe current were caused by the probe being hit, or sprayed, by charged collision fragments, formed by primary dust particles impacting on the payload body in front of the UiT

  • For some payload rotation angles, the current measured with the UiT dust probe on the ECOMA-4 rocket was up to twice that measured with the IAP dust probe, despite the IAP probe having had a collecting area that was about 4 times larger than that of the UiT probe

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Summary

Introduction

Polar Mesospheric Summer Echoes (PMSEs) are radar features formed near the mesopause (e.g. Rapp and Lubken, 2004). Havnes et al (2009) showed that when the coning angle is small, measurements made at the second grid and bottom plate of the DUSTY probe allow the current associated with the primary charge carried by the impacting particles to be distinguished from the current arising due to secondary charging. Taking into account the large coning angle, Havnes and Næsheim (2007) found that the observed magnitude and variation, as the payload rotated, of the dust current are consistent with impacting dust particles fragmenting and many of the fragments carrying away an electron each from the grid surface. We discuss the conditions under which the differences between the currents measured with the UiT probe and the IAP probe could be due to such a spray of charged fragments, and whether the measurements of the currents obtained with the two probes provide support for the large secondary charging efficiency inferred by Havnes et al (1996, 2009) and Havnes and Næsheim (2007)

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