A new analytical simulation code of acoustic-gravity waves of seismic origin and rapid co-seismic thermospheric disturbance energetics

HIGHLIGHTS

• What: This study focuses on the acoustic wave modes to understand the origin of rapid CSTDs. The consistent ray-tracing simulation in this study validates the AGW energetics in altitude-varying sound profiles, as presented in Figures 2 and 3. The simulation of ionoquakes is beyond the scope of the present study, and the authors aim to present it in a separate study. The study aims to simulate co-seismic atmospheric disturbances, estimate their formation time at thermospheric heights, and compare these estimations with ray-tracing estimations.
• Who: Saul A. Sanchez and Esfhan A. Kherani . . .
  

   

  

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