Abstract
A cosmic dust monitor for use onboard a spacecraft is currently being developed using a piezoelectric lead zirconate titanate element (PZT). Its characteristics of the PZT sensor is studied by ground-based laboratory impact experiments using hypervelocity particles supplied by a Van de Graaff accelerator. The output signals obtained from the sensor just after the impact appeared to have a waveform that was explicitly related to the particle's impact velocity. For velocities less than ∼6 km/s, the signal showed an oscillation pattern and the amplitude was proportional to the momentum of the impacting particle. For higher velocities, the signal gradually changed to a single waveform. The rise time of this single waveform was proportional to the particle's velocity for velocities above ∼6 km/s. The present paper reports on results for the low velocity case and especially discusses the effect of an outer coating of the sensor with a paint, which is used to reduce heating by solar radiation.
Original language | English |
---|---|
Pages (from-to) | 905-909 |
Number of pages | 5 |
Journal | Advances in Space Research |
Volume | 43 |
Issue number | 6 |
DOIs | |
Publication status | Published - 2009 Mar 16 |
Keywords
- BepiColombo mission
- Cosmic dust
- Dust detector
- Lead zirconate titanate (PZT)
- Mercury Dust Monitor (MDM)
- Piezoelectricity
ASJC Scopus subject areas
- Aerospace Engineering
- Space and Planetary Science