Determining spatio-temporal characteristics of coseismic travelling ionospheric disturbances (CTID) in near real-time.

Sci Rep

CNRS UMR 7154, Institut de Physique du Globe de Paris (IPGP), Université de Paris, 35-39 Rue Hélène Brion, 75013, Paris, France.

Published: October 2021

AI Article Synopsis

  • Researchers have developed a novel method to automatically detect co-seismic travelling ionospheric disturbances (CTID) in GNSS data, enabling real-time analysis within 15 minutes of an earthquake.
  • The method allows for the determination of CTID's velocity and direction, helping to understand their evolution and estimate their source location shortly after seismic events.
  • Applied to significant earthquakes in 2011, the method shows most effectiveness with high-rate 1 Hz data and can potentially be extended to analyze other types of ionospheric disturbances caused by various geophysical phenomena.

Article Abstract

Earthquakes are known to generate ionospheric disturbances that are commonly referred to as co-seismic travelling ionospheric disturbances (CTID). In this work, for the first time, we present a novel method that enables to automatically detect CTID in ionospheric GNSS-data, and to determine their spatio-temporal characteristics (velocity and azimuth of propagation) in near-real time (NRT), i.e., less than 15 min after an earthquake. The obtained instantaneous velocities allow us to understand the evolution of CTID and to estimate the location of the CTID source in NRT. Furthermore, also for the first time, we developed a concept of real-time travel-time diagrams that aid to verify the correlation with the source and to estimate additionally the propagation speed of the observed CTID. We apply our methods to the Mw7.4 Sanriku earthquake of 09/03/2011 and the Mw9.0 Tohoku earthquake of 11/03/2011, and we make a NRT analysis of the dynamics of CTID driven by these seismic events. We show that the best results are achieved with high-rate 1 Hz data. While the first tests are made on CTID, our method is also applicable for detection and determining of spatio-temporal characteristics of other travelling ionospheric disturbances that often occur in the ionosphere driven by many geophysical phenomena.

Download full-text PDF

Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC8531289PMC
http://dx.doi.org/10.1038/s41598-021-99906-5DOI Listing

Publication Analysis

Top Keywords

ionospheric disturbances
16
spatio-temporal characteristics
12
travelling ionospheric
12
determining spatio-temporal
8
ctid
8
disturbances ctid
8
ionospheric
5
characteristics coseismic
4
coseismic travelling
4
disturbances
4

Similar Publications

This study demonstrates a rich complexity of the time-frequency ionospheric signal spectrum, dependent on the measurement type and platform. Different phenomena contributing to satellite-derived and ground-derived geophysical data that only selected signal bands can be potentially sensitive to seismicity over time, and they are applicable in lithosphere-atmosphere-ionosphere coupling (LAIC) studies. In this study, satellite-derived and ground-derived ionospheric observations are filtered by a Fourier-based band-pass filter, and an experimental selection of potentially sensitive frequency bands has been carried out.

View Article and Find Full Text PDF
Article Synopsis
  • This study analyzes the response of the Brazilian ionosphere to geomagnetic storms driven by Corotating Interaction Regions (CIR) and High-Speed Solar Wind Streams (HSS) during 2016-2017.
  • It investigates Vertical Total Electron Content (VTEC) variations across three regions: equatorial, northern crest, and southern crest of the Equatorial Ionization Anomaly, noting both enhancements and depletions of up to 30 and 20 TECu, respectively.
  • The research also highlights the timing of these variations, the role of electric fields in the ionosphere, and includes new catalogs for low-latitude ionospheric storms useful for space weather and modeling.
View Article and Find Full Text PDF

One of the most intense geomagnetic storms of recent times occurred on 10-11 May 2024. With a peak negative excursion of Sym-H below -500 nT, this storm is the second largest of the space era. Solar wind energy transferred through radiation and mass coupling affected the entire Geospace.

View Article and Find Full Text PDF

We use the TIEGCM-NG nudged by MAGIC gravity waves to study the impacts of a severe thunderstorm system, with a hundred tornado touchdowns, on the ionospheric and thermospheric disturbances. The generated waves induce a distinct concentric ring pattern on GNSS TIDs with horizontal scales of 150-400 km and phase speeds of 150-300 m/s, which is well simulated by the model. The waves show substantial vertical evolution in period, initially dominated by 0.

View Article and Find Full Text PDF

During the second recovery phase of the 13-14 March 2022 storm, intense high-latitude neutral mass density spikes are detected by satellites at ∼500 km in both hemispheres. These density spikes, accurately modeled by the Global Ionospheric Thermosphere Model (GITM), are identified as high-latitude neutral mass density anomalies (HDAs). The GITM simulation indicates that these HDAs, which extends over the polar region, are important features in high-latitude neutral density.

View Article and Find Full Text PDF

Want AI Summaries of new PubMed Abstracts delivered to your In-box?

Enter search terms and have AI summaries delivered each week - change queries or unsubscribe any time!