EGU21-15151
https://doi.org/10.5194/egusphere-egu21-15151
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

An innovative methodology for locating ionosphere layer height: case study on 2011 Tohoku-Oki earthquake and tsunami

Michela Ravanelli1 and Giovanni Occhipinti2
Michela Ravanelli and Giovanni Occhipinti
  • 1Sapienza University of Rome, Geodesy and Geomatics Division, Department of Civil, Constructional and Environmental Engineering, Rome, Italy (michela.ravanelli@uniroma1.it)
  • 22Université de Paris, Institut de Physique du Globe de Paris, CNRS, F-75005 Paris, France

One of the main issues in GNSS ionosphere seismology is to localize the exact height of the single thin layer (Hion) with which the ionosphere is approximated. Hion is generally assumed to be the altitude of the maximum ionospheric ionization (hmF2), i.e., in the ionospheric F-layer. In this sense, Hion is often  be presumed from physical principles or ionospheric models. The determination of  Hion is, therefore, fundamental since it affects the coordinates of the ionospheric pierce point (IPP) and subsequentely of the sub-ionospheric pierce point (SIP).

In this work, we present a new developed methodology to determine the exact localization of Hion. We tested this approach on the TIDs (Travelling ionospheric disturbances) connected with the 2011 Tohoku-Oki earthquake and tsunami [1]. In detail, we computed the slant Total Electron Content (sTEC) variations at different Hion (in the range from 100 to 600 km) with the VARION (Variometric Approach for Real-Time Ionosphere Observation) algorithm [2,3], then we interpolated the different pattern in sTEC values related to different waves detected in the ionosphere (AGWepi, IGWtsuna and AWRayleigh) finding the mean velocity value of these waves. Subsequentely, the minimized difference between the estimated propagation velocity and the values from physical models fix us the correct Hion.

Our results show a Hion of 370 km, while ionopshere model IRI 2006 located the maximum of ionospheric ionization at an height of 270 km. This difference is important to understand how a different Hion can impact on the location of the sTEC perturbation, affecting the shape and the extent of the source from TEC observations.

 

 

 

 

References

[1] https://earthquake.usgs.gov/earthquakes/eventpage/official20110311054624120_30/executive

[2] Giorgio Savastano, Attila Komjathy, Olga Verkhoglyadova, Augusto Mazzoni, Mattia Crespi, Yong Wei, and Anthony J Mannucci, “Real-time detection of tsunami ionospheric disturbances with a stand-alone gnss receiver: A preliminary feasibility demonstration, ”Scientific reports, vol. 7, pp. 46607, 2017.

[3] Giorgio Savastano, Attila Komjathy, Esayas Shume, Panagiotis Vergados, Michela Ravanelli, Olga Verkhoglyadova, Xing Meng, and Mattia Crespi, “Advantages of geostationary satellites for ionospheric anomaly studies: Ionospheric plasma depletion following a rocket launch,”Remote Sensing, vol. 11, no. 14, pp. 1734, 2019

How to cite: Ravanelli, M. and Occhipinti, G.: An innovative methodology for locating ionosphere layer height: case study on 2011 Tohoku-Oki earthquake and tsunami, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-15151, https://doi.org/10.5194/egusphere-egu21-15151, 2021.

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