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The Polarization of Ambient Noise on Mars

Stutzmann, E. ; Schimmel, M. ; Lognonné, P. ; [weitere]

American Geophysical Union (AGU) ; 2021

In: Journal of Geophysical Research: Planets Vol. 126, No. 1 ( 2021-01)

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In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 126, No. 1 ( 2021-01)

Kurzfassung: Seismic noise on Mars is polarized horizontally at low frequency (0.03–0.3 Hz) and vertically at high frequency (0.3–1 Hz) Polarization azimuth varies with local hour and season and follows the wind direction during the day Day polarization can partly be explained by pressure or acoustic emission and seismic wavefield may only be identified in the evening

Materialart: Online-Ressource

ISSN: 2169-9097 , 2169-9100

URL: Article

DOI: 10.1029/2020JE006545

Sprache: Englisch

Verlag: American Geophysical Union (AGU)

Publikationsdatum: 2021

ZDB Id: 1086497-0

ZDB Id: 3094268-8

ZDB Id: 2016810-X

SSG: 16,13