Abstract

Abstract The 11 April 2012 East Indian Ocean earthquake is unique because of its largest ever recorded aftershock. The main earthquake occurred with a magnitude of 8.6 Mw and was followed by a strong aftershock (8.2 Mw). Our analysis of the main shock indicates that the rupture was a mixture of strike-slip and thrust faults, and significant vertical surface displacements were observed during the event. The prime interest here is to study the post-seismic ionospheric disturbances, along with their characteristics. As both earthquakes had large magnitudes, they provided an opportunity to minimize the ambiguity in identifying the corresponding seismic-induced ionospheric disturbances. Approximately 10 min after both seismic events, the nearby ionosphere started to manifest electron density perturbations that were investigated using GPS-TEC measurements. The epicenters of both events were located south of the magnetic equator, and it is believed that the varying magnetic field inclination might be responsible for the observed north-south asymmetry in the post-seismic total electron content (TEC) disturbances. These disturbances are observed to propagate up to approximately 1,500 km towards the north side of the epicenter and up to only a few hundred kilometers on the south side. The frequency analysis of the post-seismic TEC disturbances after both earthquakes exhibits the dominant presence of acoustic frequencies varying between approximately 4.0 to 6.0 mHz. The estimated propagation velocities of the post-seismic TEC disturbances during the main shock (0.89 km/s) and aftershock (0.77 km/s) confirm the presence of an acoustic frequency as the generative mode for the observed TEC fluctuations.

Highlights

  • The origin of perturbations in ionospheric electron density can be traced to various sources

  • We investigate various characteristics of post-seismic ionospheric disturbances associated with the Indian Ocean doublet earthquake that occurred on 11 April 2012

  • To confirm that the observed total electron content (TEC) fluctuations on April 11 were due to the twin seismic activity, the differential TEC variations at one of the Sumatran GPS Array (SuGAr) stations, umlh, as observed by pseudo random number (PRN) 32, were examined

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Summary

Introduction

The origin of perturbations in ionospheric electron density can be traced to various sources. Seismic activity is one of the potential sources that can affect the ionospheric electron density at smaller scales prior to, during, or after an earthquake occurrence (e.g., Liu et al 2010; Rolland et al 2011a, Rolland et al 2011b; Astafyeva et al 2013). These electron density variations are, respectively, known as pre-, co-, and post-seismic ionospheric disturbances. While propagating away from the epicenter, it generates acoustic wave perturbations that reach ionospheric altitudes and create electron density variations. It is conjectured that tsunami waves in the ocean generate gravity waves that propagate obliquely upwards and interact with the ionospheric electron density

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