Acoustic Signals of a Meteoroid Recorded on a Large-NSeismic Network and Fiber-Optic Cables

Author:

Vera Rodriguez Ismael12ORCID,Isken Marius P.34ORCID,Dahm Torsten34ORCID,Lamb Oliver D.56ORCID,Wu Sin-Mei7ORCID,Kristjánsdóttir Sigríður8ORCID,Jónsdóttir Kristín8ORCID,Sanchez-Pastor Pilar6ORCID,Clinton John7ORCID,Wollin Christopher3ORCID,Baird Alan F.9ORCID,Wuestefeld Andreas9,Booz Beat10,Eibl Eva P. S.4ORCID,Heimann Sebastian4ORCID,Goertz-Allmann Bettina P.9ORCID,Jousset Philippe3ORCID,Oye Volker9ORCID,Hjörleifsdóttir Vala11ORCID,Obermann Anne7ORCID

Affiliation:

1. 1Formerly at, NORSAR, Kjeller, Norway

2. 2Silixa LLC, Missoula, Montana, U.S.A.

3. 3GFZ German Research Centre for Geosciences, Potsdam, Germany

4. 4University of Potsdam, Institute of Geosciences, Potsdam, Germany

5. 5Department of Earth, Marine and Environmental Sciences, University of North Carolina at Chapel Hill, Chapel Hill, North Carolina, U.S.A.

6. 6Te Pū Ao | GNS Science, Wairakei Research Centre, Taupō, New Zealand

7. 7Swiss Seismological Service, ETH Zurich, Zurich, Switzerland

8. 8Icelandic Meteorological Office, Reykjavík, Iceland

9. 9NORSAR, Kjeller, Norway

10. 10Department for Meteor and Fireball Calculations, Swiss Fachgruppe Meteorastronomie, Frick, Switzerland

11. 11Reykjavík Energy, Reykjavík, Iceland

Abstract

AbstractA common challenge in acoustic meteoroid signal analyses is to discriminate whether the observed wavefield can be better described by line-source or point-source models. This challenge typically arises from a sparse availability of observations. In this work, we present an outstanding record of ground-coupled waves from local large-N seismic and distributed acoustic sensing (DAS) observations of a meteoroid in Iceland. Our complete data set includes additional regional stations located within 300 km of the meteoroid’s trajectory. The dense large-N and DAS data allow identification of acoustic phases that are almost impossible to discriminate on sparser networks, including a weak late arrival resolved mostly only by DAS. Using this data set with a new Bayesian inversion model, we estimate the trajectory parameters of one fragment from the meteoroid. With these results we investigate its orbit in the solar system and propose a classification of the Icelandic event as a slow meteoroid of asteroidal origin with an energy on the order of 4–40 GJ, a probable size on the order of centimeters, and an orbit range consistent with the main asteroid belt.

Publisher

Seismological Society of America (SSA)

Subject

Geophysics

Reference59 articles.

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