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Calibration of a Dust Scattering Instrument Using Tomographic Techniques and Its Application to a Dust Sensor

David Santalices1,2, Mateo Martínez-García1, Jesús Belmar1

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Summary

A new method characterizes Martian dust by mapping its interaction volume using experimental data and tomography. This improves understanding of Martian climate and reduces simulation time for dust sensor instruments.

Keywords:
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Area of Science:

  • Planetary Science
  • Atmospheric Science
  • Optical Engineering

Background:

  • Understanding Martian dust is crucial for Mars climate studies.
  • Existing methods for dust characterization often rely on assumptions.
  • A Dust Sensor instrument uses scattering properties to determine dust parameters.

Purpose of the Study:

  • To present a novel methodology for calculating an instrumental function for a Martian Dust Sensor.
  • To enable solving the direct problem of predicting instrument signals based on particle distribution.
  • To experimentally map the dust sensor's interaction volume.

Main Methods:

  • Utilized experimental data from a Lambertian reflector introduced into the interaction volume.
  • Applied tomography techniques, specifically the inverse Radon transform.
  • Acquired a complete experimental mapping of the interaction volume, determining the Wf function.

Main Results:

  • Successfully developed and applied a novel methodology for instrumental function calculation.
  • The method experimentally maps the interaction volume without idealizations.
  • Demonstrated the method's application in a specific case study.

Conclusions:

  • The novel methodology accurately characterizes the Dust Sensor's interaction volume.
  • This approach enhances the understanding of Martian dust properties and climate.
  • The method reduces the need for extensive simulations and avoids prior assumptions.