Improving Constraints on Planetary Interiors With PPs Receiver Functions.

InSight Mars Martian crust Receiver function Seismology Transdimensional hierarchical Bayesian

Journal

Journal of geophysical research. Planets
ISSN: 2169-9097
Titre abrégé: J Geophys Res Planets
Pays: United States
ID NLM: 101661797

Informations de publication

Date de publication:
Nov 2021
Historique:
received: 29 06 2021
revised: 06 10 2021
accepted: 12 10 2021
entrez: 26 11 2021
pubmed: 27 11 2021
medline: 27 11 2021
Statut: ppublish

Résumé

Seismological constraints obtained from receiver function (RF) analysis provide important information about the crust and mantle structure. Here, we explore the utility of the free-surface multiple of the P-wave (PP) and the corresponding conversions in RF analysis. Using earthquake records, we demonstrate the efficacy of PPs-RFs before illustrating how they become especially useful when limited data is available in typical planetary missions. Using a transdimensional hierarchical Bayesian deconvolution approach, we compute robust P-to-S (Ps)- and PPs-RFs with

Identifiants

pubmed: 34824966
doi: 10.1029/2021JE006983
pii: JGRE21764
pmc: PMC8597591
doi:

Types de publication

Journal Article

Langues

eng

Pagination

e2021JE006983

Informations de copyright

© 2021. The Authors.

Références

Science. 2021 Jul 23;373(6553):438-443
pubmed: 34437117
Space Sci Rev. 2019;215(1):12
pubmed: 30880848
Science. 2013 Feb 8;339(6120):671-5
pubmed: 23223394
Science. 1999 May 28;284(5419):1495-503
pubmed: 10348732
Science. 2021 Jul 23;373(6553):434-438
pubmed: 34437116
Science. 1998 May 22;280(5367):1232-5
pubmed: 9596570
Science. 2021 Jul 23;373(6553):443-448
pubmed: 34437118
Science. 1973 Jun 8;180(4090):1063-4
pubmed: 17806584
Science. 2011 Jan 21;331(6015):309-12
pubmed: 21212323

Auteurs

D Kim (D)

Department of Geology University of Maryland College Park College Park MD USA.
Institute of Geophysics ETH Zürich Zürich Switzerland.

V Lekić (V)

Department of Geology University of Maryland College Park College Park MD USA.

J C E Irving (JCE)

School of Earth Sciences University of Bristol Bristol UK.

N Schmerr (N)

Department of Geology University of Maryland College Park College Park MD USA.

B Knapmeyer-Endrun (B)

Bensberg Observatory University of Cologne Cologne Germany.

R Joshi (R)

Max Planck Institute for Solar System Research Göttingen Germany.

M P Panning (MP)

Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA.

B Tauzin (B)

Université de Lyon UCBL ENSL CNRS LGL-TPE Villeurbanne France.
Research School of Earth Sciences Australian National University Acton ACT Australia.

F Karakostas (F)

Department of Geology University of Maryland College Park College Park MD USA.
Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Bologna Bologna Italy.

R Maguire (R)

Department of Geology University of Maryland College Park College Park MD USA.
Department of Computational Mathematics, Science, and Engineering Michigan State University East Lansing MI USA.

Q Huang (Q)

Department of Geology University of Maryland College Park College Park MD USA.
Department of Physics New Mexico State University Las Cruces NM USA.

S Ceylan (S)

Institute of Geophysics ETH Zürich Zürich Switzerland.

A Khan (A)

Institute of Geophysics ETH Zürich Zürich Switzerland.

D Giardini (D)

Institute of Geophysics ETH Zürich Zürich Switzerland.

M A Wieczorek (MA)

Université Côte d'Azur Observatoire de la Côte d'Azur CNRS Laboratoire Lagrange Nice France.

P Lognonné (P)

Université de Paris Institut de Physique du Globe de Paris CNRS Paris France.

W B Banerdt (WB)

Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA.

Classifications MeSH