ArticleNature2022
In situ recording of Mars soundscape.
Erratum issuedAbstract read
In one paragraph
Article in Nature, 2022. The graph could read no effect estimate from its abstract, so it casts no vote on the map. An erratum has been issued. Cited by 8 papers.
0numbers the graph read from it
0cells of the map it votes in
8citing papers in PubMed
–field-weighted citation impact
What it found
Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.
The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.
The trial behind it
Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.
Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.
Who cites it
8 citing papers in PubMed.
- Article
- Speed of sound for understanding metals in extreme environments.Applied physics reviews · 2024Article
- An estimate of the impact rate on Mars from statistics of very-high-frequency marsquakes.Nature astronomy · 2024Article
- Spectral location for the universal scaling regime in Martian atmospheric turbulence.Communications earth & environment · 2024Article
- Lifting and Transport of Martian Dust by the Ingenuity Helicopter Rotor Downwash as Observed by High-Speed Imaging From the Perseverance Rover.Journal of geophysical research. Planets · 2022Article
- Geological, multispectral, and meteorological imaging results from the Mars 2020 Perseverance rover in Jezero crater.Science advances · 2022Article
- Dust, Sand, and Winds Within an Active Martian Storm in Jezero Crater.Geophysical research letters · 2022Article
- Article
Corrections and comments
- Commented on by
- Erratum issued
Authors and funding
43 authors.
S MauriceInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France. sylvestre.maurice@irap.omp.eu.ORCID http://orcid.org/0000-0001-5702-8002
B ChideSpace and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM, USA. bchide@lanl.gov.ORCID http://orcid.org/0000-0002-5124-9119
N MurdochInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France.ORCID http://orcid.org/0000-0002-9701-4075
R D LorenzSpace Exploration Sector, Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA.
D MimounInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France.ORCID http://orcid.org/0000-0002-3427-2974
R C WiensSpace and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM, USA.ORCID http://orcid.org/0000-0002-3409-7344
A StottInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France.
X JacobInstitut de Mécanique des Fluides, Université de Toulouse 3 Paul Sabatier, INP, CNRS, Toulouse, France.ORCID http://orcid.org/0000-0001-6718-4981
T BertrandLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, CNRS, Sorbonne Université, Université Paris Diderot, Meudon, France.ORCID http://orcid.org/0000-0002-2302-9776
F MontmessinLaboratoire Atmosphères, Milieux, Observations Spatiales, CNRS, Université Saint-Quentin-en-Yvelines, Sorbonne Université, Guyancourt, France.ORCID http://orcid.org/0000-0002-4187-1457
N L LanzaSpace and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM, USA.ORCID http://orcid.org/0000-0003-4445-7996
C Alvarez-LlamasUniversidad de Málaga, Málaga, Spain.ORCID http://orcid.org/0000-0001-7793-7000
S M AngelDepartment of Chemistry and Biochemistry, University of South Carolina, Columbia, SC, USA.
M AungJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
J BalaramJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
O BeyssacInstitut de Minéralogie, de Physique des Matériaux et de Cosmochimie, CNRS, Sorbonne Université, MNHN, Paris, France.
A CousinInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.
G DeloryHeliospace Corporation, Berkeley, CA, USA.
O ForniInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.ORCID http://orcid.org/0000-0001-6772-9689
T FouchetLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, CNRS, Sorbonne Université, Université Paris Diderot, Meudon, France.ORCID http://orcid.org/0000-0001-9040-8285
O GasnaultInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.ORCID http://orcid.org/0000-0002-6979-9012
H GripJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
M HechtHaystack Observatory, Massachusetts Institute of Technology, Westford, MA, USA.ORCID http://orcid.org/0000-0002-4114-4583
J HoffmanDepartment of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA, USA.
J LasernaUniversidad de Málaga, Málaga, Spain.
J LasueInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.ORCID http://orcid.org/0000-0001-9082-4457
J MakiJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
J McCleanHaystack Observatory, Massachusetts Institute of Technology, Westford, MA, USA.
P-Y MeslinInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.ORCID http://orcid.org/0000-0002-0703-3951
S Le MouélicLaboratoire de Planétologie et Géosciences, CNRS, Nantes Université, Université Angers, Nantes, France.ORCID http://orcid.org/0000-0001-5260-1367
A MunguiraEscuela de Ingeniería de Bilbao, Universidad del País Vasco UPV/EHU, Bilbao, Spain.ORCID http://orcid.org/0000-0002-1677-6327
C E NewmanAeolis Corporation, Sierra Madre, CA, USA.ORCID http://orcid.org/0000-0001-9990-8817
J A Rodríguez ManfrediCentro de Astrobiología (INTA-CSIC), Madrid, Spain.ORCID http://orcid.org/0000-0003-0461-9815
J MorosUniversidad de Málaga, Málaga, Spain.
A OllilaSpace and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM, USA.
P PilleriInstitut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, CNES, Toulouse, France.
S SchröderDeutsches Zentrum für Luft- und Raumfahrt (DLR), Institute of Optical Sensor Systems, Berlin, Germany.ORCID http://orcid.org/0000-0003-1870-3663
M de la Torre JuárezJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.ORCID http://orcid.org/0000-0003-1393-5297
T TzanetosJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
K M StackJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
K FarleyJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
K WillifordJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.ORCID http://orcid.org/0000-0003-0633-408X
SuperCam team
Funding
No grant is acknowledged in the PubMed record.
Abstract
Before the Perseverance rover landing, the acoustic environment of Mars was unknown. Models predicted that: (1) atmospheric turbulence changes at centimetre scales or smaller at the point where molecular viscosity converts kinetic energy into heat
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