Low-Frequency Atmospheric Gravity Waves from Vertical Tectonic Deformation During Two Recent Chilean Megathrust Events: the 2010 Maule (Mw8.8), and 2014 Iquique (Mw8.2) Earthquakes

Takeshi Mikumo1, *, Takuo Shibutani2, Makiko Iwakuni3, Nobuo Arai4
1 Kyoto University, Uji, Kyoto 611-0001, Japan,
2 Disaster Prevention Research Institute, Kyoto University, Uji, Kyoto 611-0001, Japan
3 Japan Weather Association, Tokyo 170-6045, Japan
4 Disaster Mitigation Research Center, Nagoya University, Nagoya 464-8601, Japan

Article Metrics

CrossRef Citations:
Total Statistics:

Full-Text HTML Views: 1488
Abstract HTML Views: 943
PDF Downloads: 485
ePub Downloads: 270
Total Views/Downloads: 3186
Unique Statistics:

Full-Text HTML Views: 667
Abstract HTML Views: 532
PDF Downloads: 298
ePub Downloads: 182
Total Views/Downloads: 1679

© 2017 Mikumo et al.

open-access license: This is an open access article distributed under the terms of the Creative Commons Attribution 4.0 International Public License (CC-BY 4.0), a copy of which is available at: This license permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

* Address correspondence to this author at the Kyoto University, Uji, Kyoto 611-0001, Japan; Tel/Fax: +8-774-32-0072; E-mail:



Low-frequency atmospheric waves with gravity modes were recorded within 6.5 hours and 4.7 hours after two recent Chilean megathrust events, the 2010 Maule (Mw = 8.8), and 2014 Iquique (Mw = 8.2) earthquakes, respectively, at several microbarograph stations of the International Monitoring System (IMS) in South America and its surrounding regions.


Their apparent phase velocity up to the epicentral distances of 7,404 km and 6,481 km was found to be around 319 m/s and 337 m/s, respectively for the gravity modes after the two earthquakes. We tried to construct synthetic waveforms to be recorded at some of these microbarograph stations, incorporating various seismic source characteristics of the two earthquakes, and also a standard sound velocity structure up to a height of 220 km above the ground surface. The comparison appears to show some agreement between the observed and synthetic waveforms at least for the first 22 min for appropriate combinations of these source parameters.


The results indicate that the observed atmospheric gravity waves at the initial stage appear to have actually been excited at the source region of these megathrust earthquakes.


The average rise time of vertical tectonic movement at the source region, which is estimated to be from the observed gravity waves, appears to be in the range between 2 and 3 min.

Keywords: Atmospheric gravity waves, Coseismic vertical deformation, The 2010 Maule and 2014 Iquique, Chilean megathrust earthquakes.