Development and testing of the MicroMED sensor: From BreadBoard model to flight model
Journal
Date Issued
2024
Author(s)
Abstract
Suspended dust plays a critical role in regulating the Martian climate by influencing the atmospheric thermal gradient, altering the
amount of infrared and visible energy absorbed and scattered by the atmosphere, and acting as condensation nuclei for CO2 iceclouds
particles. There are many well demonstrated, dust-related effects on martian climate which depend on dustsize, concentration,
chemical and bulk composition. Currently, an accurate estimation of these parameters is lacking as they are derived from indirect measurement
of the optical depth acquired from the surface and orbital data. These indirect measurements require a priori assumptions on
the grain distribution curve and are hence subject to possible biases. To overcome these limitations, an optical particles counter called
MicroMED has been developed under the National Institute of Astrophysics (INAF) leadership. MicroMED can measure the sizes of
individual dust grains in a specific volume of air thus providing the grain size distribution and concentration. MicroMED has been
selected to join the Dust Complex payload on board the ExoMars 2022. The Flight Model of the instrument has been developed and
optimized starting from two prototype BreadBoard versions. Here we present the sub-systems that constitute MicroMED and their testing
and characterization process, performed using the Breadboard models. We discuss the optimizations and improvements introduced
on the basis of the prototype results and the overall performances of the final design.
Issn Identifier
0273-1177
Rights
open.access
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