An acoustic investigation of the near-surface turbulence on Mars.


Journal

The Journal of the Acoustical Society of America
ISSN: 1520-8524
Titre abrégé: J Acoust Soc Am
Pays: United States
ID NLM: 7503051

Informations de publication

Date de publication:
01 Jan 2024
Historique:
received: 04 10 2023
accepted: 14 12 2023
medline: 19 1 2024
pubmed: 19 1 2024
entrez: 19 1 2024
Statut: ppublish

Résumé

The Perseverance rover is carrying out an original acoustic experiment on Mars: the SuperCam microphone records the spherical acoustic waves generated by laser sparks at distances from 2 m to more than 8 m. These N-shaped acoustic waves scatter from the multiple local heterogeneities of the turbulent atmosphere. Therefore, large and random fluctuations of sound travel time and intensity develop as the waves cross the medium. The variances of the travel times and the scintillation index (normalized variance of the sound intensity) are studied within the mathematical formalism of the propagation of spherical acoustic waves through thermal turbulence to infer statistical properties of the Mars atmospheric temperature fluctuation field. The comparison with the theory is made by simplifying assumptions that do not include wind fluctuations and diffraction effects. Two Earth years (about one Martian year) of observations acquired during the maximum convective period (10:00-14:00 Mars local time) show a good agreement between the dataset and the formalism: the travel time variance diverges from the linear Chernov solution exactly where the density of occurrence of the first caustic reaches its maximum. Moreover, on average, waves travel faster than the mean speed of sound due to a fast path effect, which is also observed on Earth. To account for the distribution of turbulent eddies, several power spectra are tested and the best match to observation is obtained with a generalized von Karman spectrum with a shallower slope than the Kolmogorov cascade, ϕ(k)∝(1+k2L2)-4/3. It is associated with an outer scale of turbulence, L, of 11 cm at 2 m above the surface and a standard deviation of 6 K over 9 s for the temperature. These near-surface atmospheric properties are consistent with a weak to moderate wave scattering regime around noon with little saturation. Overall, this study presents an innovative and promising methodology to probe the near-surface atmospheric turbulence on Mars.

Identifiants

pubmed: 38240669
pii: 3037488
doi: 10.1121/10.0024347
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

420-435

Informations de copyright

© 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).

Auteurs

Baptiste Chide (B)

Space and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA.

Philippe Blanc-Benon (P)

Laboratoire de Mécanique des Fluides et d'Acoustique, Centre National de la Recherche Scientifique, Ecole Centrale de Lyon, Institut National des sciences appliquées Lyon, Université Lyon 1, Ecully, France.

Tanguy Bertrand (T)

Laboratoire d'études spatiales et d'instrumentation en astrophysique, Observatoire de Paris, Université Paris Sciences & Lettres, Sorbonne Université, Centre National de la Recherche Scientifique, Meudon, France.

Xavier Jacob (X)

Institut de Mécanique des Fluides de Toulouse, Université Toulouse 3, Institut National Polytechnique, Centre National de la Recherche Scientifique, Toulouse, France.

Jérémie Lasue (J)

Institut de Recherche en Astrophysique et Planétologie, Université Toulouse 3, Centre National de la Recherche Scientifique, Centre National d'Etudes Spatiales, Toulouse, France.

Ralph D Lorenz (RD)

Space Exploration Sector, Johns Hopkins Applied Physics Laboratory, Laurel, Maryland 20723, USA.

Franck Montmessin (F)

Laboratoire Atmosphères Observations Spatiales, Centre National de la Recherche Scientifique, Université Saint-Quentin-en-Yvelines, Sorbonne Université, Guyancourt, France.

Naomi Murdoch (N)

Institut Supérieur de l'Aeronautique et de l'Espace, Université de Toulouse, Toulouse, France.

Jorge Pla-Garcia (J)

Centro de Astrobiologia, Madrid, Spain.

Fabian Seel (F)

Institute of Optical Sensor Systems, German Aerospace Center, Berlin, Germany.

Susanne Schröder (S)

Institute of Optical Sensor Systems, German Aerospace Center, Berlin, Germany.

Alexander E Stott (AE)

Institut Supérieur de l'Aeronautique et de l'Espace, Université de Toulouse, Toulouse, France.

Manuel de la Torre Juarez (M)

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA.

Roger C Wiens (RC)

Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, Indiana 47907, USA.

Classifications MeSH