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- Title
Geographical, Seasonal and Diurnal Variations of Acoustic Attenuation, and Sound Speed in the Near‐Surface Martian Atmosphere.
- Authors
Gillier, Martin; Petculescu, Andi; Murdoch, Naomi; Stott, Alexander E.; Gerier, Solène; Maurice, Sylvestre; Mimoun, David
- Abstract
This work introduces a comprehensive model of sound attenuation and speed on Mars, in light of the recent operation of several microphones on the surface of Mars. The proposed acoustic model calculates the sound speed and attenuation throughout the near‐surface Martian atmosphere based on first‐principles. We evaluate the effects of the seasonal and diurnal cycle of air temperature, pressure and CO2, as well as the concentration of airborne dust on the sound attenuation. The attenuation and speed of sound are most sensitive to the air temperature and, therefore, they vary with the diurnal temperature cycle and to a lesser degree with the seasonal changes in temperature. The speed of sound also varies with the seasonal variations of the concentration of CO2. The main outcome of this work is an acoustic model capable of computing the sound speed and attenuation for any location at the Martian surface at any time of year and any time of day. Plain Language Summary: Sound offers new means of investigating the Martian environment. To study the properties of sound sources on Mars, or to derive atmospheric properties from the way sound travels in the Martian atmosphere, a model of the sound attenuation and speed on Mars is needed. In this paper, we propose such a model that allows the sound attenuation and speed at the Martian surface to be computed at any point and time. We investigate how these two properties change with air temperature, pressure, the chemical composition of the Martian atmosphere, the concentration of airborne dust, and with time of day and season. This paints the picture of Mars as a very contrasting planet acoustically, with a very wide range of attenuation and speed of sound compared to Earth because of the daily variations of temperature and the yearly variations of pressure and chemical composition. Key Points: Attenuation and speed of sound are modeled at every point of the Martian surfaceSound attenuation and speed are most affected by the variation of pressure and temperature associated with the diurnal and seasonal cyclesThe variations of sound attenuation and speed during a given day are very strong compared to Earth
- Subjects
MARTIAN atmosphere; ACOUSTICS; MARTIAN surface; ATMOSPHERIC temperature; SPEED of sound; ACOUSTIC models; ROTATION of the earth
- Publication
Journal of Geophysical Research. Planets, 2024, Vol 129, Issue 5, p1
- ISSN
2169-9097
- Publication type
Article
- DOI
10.1029/2023JE008257