Documents

Seismic waves excited before and after earthquakes can make vertical motion of the Earth’s surface. The perturbations can propagate to the middle and upper atmosphere and cause variations and oscillations of atmospheric characteristics at different altitudes. Among the mechanisms of such ionospheric perturbations could be propagation of acoustic-gravity waves (AGWs) in the atmosphere caused by seismic excitations at the Earth’s surface. In the present study, we use the recently developed nonlinear numerical Whole-altitude Acoustic-Gravity Wave Model (WAGWM) to simulate propagation of supersonic wave modes from the ground to the upper atmosphere.
Translated title of the contributionPenetration of acoustic-gravity modes from supersonic surface excitation to the upper atmosphere
Original languageRussian
Title of host publication Атмосферной Радиации и Динамике (МСАРД-2017)
Subtitle of host publicationТезисы
Place of PublicationСПб
PublisherИздательство Санкт-Петербургского университета
Pages204-206
StatePublished - 2017
Event Atmospheric radiation and dynamics - Санкт-Петербург, Russian Federation
Duration: 27 Jun 201730 Jun 2017

Conference

Conference Atmospheric radiation and dynamics
Country/TerritoryRussian Federation
CityСанкт-Петербург
Period27/06/1730/06/17

    Scopus subject areas

  • Earth and Planetary Sciences(all)

ID: 9851264