[Skip to Content]
Banner
Menu
  • Home
  • Submit Abstract
  • Home
  • 2019 Annual Meeting Session Gallery
  • The InSight Mission – Seismology on Mars and Beyond
  • Mars Structure Service: Single-Station and Single-Event Marsquake Inversion for Structure Using Synthetic Martian Waveforms

 

Mars Structure Service: Single-Station and Single-Event Marsquake Inversion for Structure Using Synthetic Martian Waveforms

Date: 4/25/2019

Time: 09:15 AM

Room: Vashon

The InSight lander successfully delivered geophysical instrument package on the Martian surface on November 26th, 2018, including a broadband and a short-period seismometer (Seismic Experiment for Interior Structure, SEIS). Routine operations are split into two services: the Mars Structure Service (MSS) and the Marsquake Service (MQS), which are responsible for defining structure models and seismicity catalogs, respectively. The first “deliverable” of the MSS will be a model based on the events detected during the first 3 months of seismic monitoring of the mission, for which only a few quakes might be expected based on current estimates of Mars seismic activity. To test our approach of determining the interior model of Mars and to prepare the InSight science team for data return, we made use of a “blind test” time series for which the Marsquake parameters (location, depth, origin time, and moment tensor) and interior model were unknown to the group at large.

In preparation for the mission, the goal was to develop mature algorithms to handle the data as efficiency as possible. Synthetic seismic waveforms were computed in a 1D mantle model with a 3D crust on top using AxiSEM and Salvus. The time series were created by adding seismic noise that relies on pre-landing estimates of noise generated by the sensors, electronic system, environment, and nearby lander.

We detail and compare the results of this “blind test” using different methods including inversion of surface wave dispersion data, body waves travel times, and the waveforms themselves. Effects of fixing mars quake location and origin time are investigated. To allow for tighter constraints, we also test the use of priors based on thermodynamically-constrained models. These techniques considered here form a large part of the planned modeling of the MSS that will be ultimately employed with the first recording of a seismic event by InSight.

 


Presenting Author: Mark P. Panning


Authors

Mark P Panning

Presenting Author Corresponding Author

mark.p.panning@jpl.nasa.gov

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States

Presenting Author
Corresponding Author

Eric Beucler

eric.beucler@univ-nantes.fr

Université de Nantes, Laboratoire de Planétologie et de Géodynamique, Nantes, , France

Mélanie Drilleau

drilleau@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Amir Khan

amir.khan@erdw.ethz.ch

ETH Zurich, Zürich, , Switzerland

Philippe Lognonné

lognonne@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Caroline Beghein

cbeghein@epss.ucla.edu

University of California, Los Angeles, Los Angeles, California, United States

Haotian Xu

htxu@ucla.edu

University of California, Los Angeles, Los Angeles, California, United States

Sabrina Menina

menina@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Salma Barkaoui

barkaoui@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Vedran Lekic

ved@umd.edu

University of Maryland, College Park, Maryland, United States

Simon Stähler

simon.staehler@erdw.ethz.ch

ETH Zurich, Zurich, , Switzerland

Martin van Driel

vandriel@erdw.ethz.ch

ETH Zurich, Zurich, , Switzerland

Balthasar Kenda

kenda@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Naomi Murdoch

naomi.murdoch@isae.fr

Institut supérieur de l'aéronautique et de l'espace, Toulouse University, Toulouse, , France

John Clinton

jclinton@sed.ethz.ch

ETH Zurich, Zurich, , Switzerland

Domenico Giardini

domenico.giardini@erdw.ethz.ch

ETH Zurich, Zurich, , Switzerland

Suzanne E Smrekar

suzanne.e.smrekar@jpl.nasa.gov

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States

Eléonore Stutzmann

stutz@ipgp.fr

Institut de Physique du Globe de Paris, Paris, , France

Martin Schimmel

schimmel@ictja.csic.es

ICTJA-CSIC, Barcelona, , Spain

Mars Structure Service: Single-Station and Single-Event Marsquake Inversion for Structure Using Synthetic Martian Waveforms

Category

The InSight Mission – Seismology on Mars and Beyond

Description