[Skip to Content]
Banner
Menu
  • Home
  • Submit Abstract
  • Home
  • 2019 Annual Meeting Session Gallery
  • The InSight Mission – Seismology on Mars and Beyond
  • SEIS: Overview, Deployment and First Science on the Ground

 

SEIS: Overview, Deployment and First Science on the Ground

Date: 4/25/2019

Time: 08:30 AM

Room: Vashon

The InSight mission landed on Mars on 11/26/2018. This is the first planetary mission deploying a complete geophysical observatory on another body than Earth after the Apollo Lunar Surface Experiments Package (ALSEP) deployed on the Moon during the Apollo program. It will provide the first ground truth constraints on interior structure of the planet. The Seismic Experiment for Interior Structure (SEIS) is one of the three primary scientific investigations, the two other ones being the Heat Flow and Physical Properties Package (HP3) and the Rotation and Interior Structure Experiment (RISE). SEIS is completed by the APSS experiment (InSight Auxiliary Payload Suite), one of which goal is to document the atmospheric source of seismic noise and signals. After a brief description of the SEIS experiment, we report the deployment process, including the evolution of the SEIS noise from on the deck measurements (with only SPs) toward on the ground (with both VBBs and SPs), without and finally with wind shield.

We compare these noise levels to those obtained on Earth during tests, to those recorded on the Moon and to those predicted prior the landing. In all configurations, we identify the contribution of the lander noise and finally discuss what might remain in term of micro-seismic background, i.e. uncoherent seismic waves background.

As proposed by several studies made prior the landing, atmospheric seismic signals on the ground are expected from turbulences in the planetary boundary layer or from dust devils, at both long period and short period. We expect also local time variation of the seismic noise as a consequence of weather activity as well as possible micro-seismic noise associated to trapped surface or body waves in the subsurface low velocity channel. We challenge these predictions with the data and discuss the events and spectrum identified with both the SEIS and APSS data. We finally compare them with modeling made with different subsurface structure.

Additional authors :

https://www.seisinsight.eu/en/public-2/seis-instrument/seis-working-groupsteam

 


Presenting Author: Philippe Lognonné


Authors

Philippe Lognonné

Presenting Author Corresponding Author

lognonne@ipgp.fr

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

Presenting Author
Corresponding Author

William B Banerdt

william.b.banerdt@jpl.nasa.gov

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

William T Pike

w.t.pike@imperial.ac.uk

Imperial College London, London, , United Kingdom

Domenico Giardini

domenico.giardini@erdw.ethz.ch

ETH Zurich, Zurich, , Switzerland

Don Banfield

banfield@astro.cornell.edu

Cornell Center for Astrophysics and Planetary Science, Ithaca, New Jersey, United States

Ulrich Christensen

christensen@mps.mpg.de

Max Planck Institute for Solar System Research, Department of Planets and Comets, Goettingen, , Germany

Marco Bierwirth

bierwirthm@mps.mpg.de

Max Planck Institute for Solar System Research, Department of Planets and Comets, Goettingen, , Germany

Simon Calcutt

calcutt@atm.ox.ac.uk

University of Oxford, Atmospheric, Oceanic, & Planetary Physics, Oxford, , United Kingdom

John Clinton

jclinton@sed.ethz.ch

Institut of Geophysics, ETHZ, Zurich, , Switzerland

Sharon Kedar

sharon.kedar@jpl.nasa.gov

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

Raphael Garcia

raphael.garcia@isae-supaero.fr

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

Sébastien de Raucourt

deraucourt@ipgp.fr

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

Kenneth Hurst

kenneth.j.hurst@jpl.nasa.gov

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

Taichi Kawamura

kawamura@ipgp.fr

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

David Mimoun

david.mimoun@isae.fr

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

Mark P Panning

mark.p.panning@jpl.nasa.gov

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

Aymeric Spiga

aymeric.spiga@sorbonne-universite.fr

LMD, Sorbonne Université, Paris, , France

Peter Zweifel

pzweifel@retired.ethz.ch

Institut of Geophysics, ETHZ, Zurich, , Switzerland

SEIS: Overview, Deployment and First Science on the Ground

Category

The InSight Mission – Seismology on Mars and Beyond

Description