Author/Authors :
S. Takechi، نويسنده , , K. Nogami، نويسنده , , T. Miyachi، نويسنده , , M. Fujii، نويسنده , , N. Hasebe، نويسنده , , T. Iwai*، نويسنده , , S. Sasaki، نويسنده , , H. Ohashi ، نويسنده , , H. Shibata، نويسنده , , E. Grün، نويسنده , , R. Srama، نويسنده , , D. N. Okada، نويسنده ,
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.
Keywords :
Cosmic dust , BepiColombo mission , Mercury Dust Monitor (MDM) , Dust detector , Piezoelectricity , Lead zirconate titanate (PZT)