JPL
Careers
Education
Science & Technology
JPL Logo
JPL Logo
Image

NASA 'Sees' Tohoku-Oki Earthquake and Tsunami in Earth's Upper Atmosphere

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ Feb. 16, 2012
This shows how waves of energy from the Tohoku-Oki earthquake and tsunami of March 11, 2011, pierced through into Earth's upper atmosphere in the vicinity of Japan, disturbing the density of electrons in the ionosphere.
Click on an individual image for larger view

This animation shows how waves of energy from the Tohoku-Oki earthquake and tsunami of March 11, 2011, pierced through into Earth's upper atmosphere in the vicinity of Japan, disturbing the density of electrons in the ionosphere. These disturbances were monitored by tracking GPS signals between satellites and ground receivers.

The disturbance measurements, known as vertical total electron content (VTEC), have been filtered to show wave-like disturbances in ionospheric electron density with frequencies between 0.5 and 5 milihertz (periods between 33 minutes and 3.3 minutes), similar to the frequency of a tsunami. The locations of the colored points in the animation correspond to the region of the ionosphere being monitored by the GPS receivers. Each receiver (there are more than 1,200 in Japan) can simultaneously receive signals from approximately 12 different GPS satellites, and hence we can monitor a wide range of locations in the ionosphere. (The motion of these Japan-shaped "clumps" is due to the motion of the GPS satellites in the sky, and is not related to the earthquake and tsunami. Rather, it is the changing color of the dots corresponding to the disturbed ionosphere.) This analysis has been done previously for the Samoa 2009 and Chile 2010 tsunamis [Galvan et al., 2011], but the Tohoku 2011 event represents the first time a major earthquake and tsunami have occurred in a region where the ionosphere over the epicenter was being observed by such a dense network of GPS receivers.

A model of ocean tsunami wavefronts [Song, 2007] is overlaid in blue to show the correlation between variations in the ionosphere above and ocean surface below. Note that traveling ionospheric disturbances (TIDs), visible throughout the animation, are correlated with the position of the tsunami. The earlier TIDs are likely associated with acoustic (longitudinal) and Rayleigh (transverse) waves caused by the earthquake itself, while later, slower-moving TIDs may be associated with atmospheric internal gravity waves caused by both the earthquake and the tsunami. The colorbar at right shows the magnitude of VTEC perturbation in the ionosphere in TECU (1 TECU = 10^12 electrons per square centimeter), while the left colorbar shows the size of the sea surface waves, in meters.

Notes of Interest:

  • The main shock of the earthquake occurs at 05:46 UT (soon after the start of the movie).
  • The earthquake disturbs the atmosphere, creating acoustic and Rayleigh waves, which propagate up to the ionosphere (reaching a peak in ionization at an altitude of 300 kilometers) within 10 minutes after the quake.
  • These fast-moving waves (1,000 meters per second for acoustic, 3,400 meters per second for Rayleigh) are visible in ionospheric Total Electron Content (TEC) measurements, as annotated in the movie.
  • The tsunami also disturbs the atmosphere, creating gravity waves that take approximately 30 to 40 minutes to reach the ionosphere. These gravity waves match the horizontal speed of the tsunami at the time they were generated, moving 200 to 300 meters per second.
  • The annotations point out gravity waves as observed in the ionosphere, sometimes aligning with the modeled ocean tsunamis (shown in blue).
  • Note the gravity waves traveling over and to the west of Japan, despite the tsunami stopping at the coast. It is likely that the gravity waves persisted in the ionosphere for some significant amount of time after the ocean waves stopped.
  • (Some noise in the measurements can be seen at very low elevation angles, meaning points that are very distant from Japan. Such noise is due to the radio waves from the GPS satellites traveling through a longer portion of the ionosphere, and being subject to the integrated ionospheric variations along that path.)

Explanation of 4-panel slide:

  • This series of four images shows several travel-time plots illustrating the observed ionospheric perturbations and modeled ocean tsunami within 1,500 kilometers of the earthquake's epicenter.
  • Figure A (upper left) shows a travel-time plot for a single satellite (SVN 55, corresponding to PRN 15) in communication with all 1,198 GPS receivers in Japan. VTEC perturbations derived from the band-pass filter technique are shown in color in units of TECU. A range of different wave speeds is visible, including Rayleigh waves (with slopes parallel to the 3,400 meters per second reference line), acoustic waves (parallel to the 1,000 meters per second line), and gravity waves with a range of different speeds between 200 and 300 meters per second. A gravity wave reference line with a slope of 240 meters per second shows an average wave speed for the Tohoku-Oki tsunami in this region, according to the model by Y. Tony Song. (Note that the reference lines will not necessarily lie directly on top of the perturbation. Rather, one should compare the slope of a perturbation to the slope of a reference line to infer the relative horizontal speed of that disturbance in the ionosphere.)
  • Figure B (upper right) is the same as Figure A, but shows data from all available satellites, not just SVN55.
  • Figure C (lower left) shows the Song tsunami model, for comparison of the wavefront on the ocean surface with the ionospheric observations.
  • Figure D (lower right) shows Figure C overlaid on Figure B. Note that for a given geographical distance from the epicenter, the ionospheric disturbances are passing by roughly 24 minutes after the ocean tsunami. This may be due to changing tsunami speeds with varying ocean depths, causing the ionospheric signature to not match the ocean tsunami position exactly at any given time, due to the time necessary for the gravity wave to reach the ionosphere.

References:

    Galvan, D. A., A. Komjathy, M. P. Hickey, and A. J. Mannucci (2011), The 2009 Samoa and 2010 Chile tsunamis as observed in the ionosphere using GPS total electron content, Journal of Geophysical Research (Space Physics), 116, A06,318, 10.1029/2010JA016204.

Song, Y. T. (2007), Detecting tsunami genesis and scales directly from coastal GPS stations, Geophys. Res. Lett., 34, L19,602, 10.1029/2007GL031681.

Download JPG
Download TIFF
Target
  • Earth
Credit
NASA/JPL-Caltech

Keep Exploring

About JPL
Who We Are
Directors
Careers
Internships
The JPL Story
JPL Achievements
Documentary Series
JPL Annual Report
Executive Council
Missions
Current
Past
Future
All
News
All
Earth
Solar System
Stars and Galaxies
Eyes on the News
Subscribe to JPL News
Galleries
Images
Videos
Audio
Podcasts
Apps
Visions of the Future
Slice of History
Robotics at JPL
Events
Lecture Series
Speakers Bureau
Calendar
Visit
Public Tours
Virtual Tour
Directions and Maps
Topics
JPL Life
Solar System
Mars
Earth
Climate Change
Exoplanets
Stars and Galaxies
Robotics
More
Asteroid Watch
NASA's Eyes Visualizations
Universe - Internal Newsletter
Social Media
Accessibility at NASA
Contact Us
Get the Latest from JPL
Follow Us

JPL is a federally funded research and development center managed for NASA by Caltech.

More from JPL
Careers
Education
Science & Technology
Acquisition
JPL Store
Careers
Education
Science & Technology
Acquisition
JPL Store
Related NASA Sites
Basics of Spaceflight
NASA Kids Science - Earth
Earth / Global Climate Change
Exoplanet Exploration
Mars Exploration
Solar System Exploration
Space Place
NASA's Eyes Visualization Project
Voyager Interstellar Mission
NASA
Caltech
Privacy
Image Policy
FAQ
Feedback
Version: v3.1.3 - 5e83a9a
Site Managers:Emilee Richardson, Alicia Cermak
Site Editors:Naomi Hartono, Steve Carney
CL#:21-0018