Analysis of Ionospheric Disturbances during X-Class Solar Flares (2021–2022) Using GNSS Data and Wavelet Analysis

The influence of solar activity on the ionosphere, a critical area of investigation due to its relevance to the Sun–Earth relationship, has been extensively examined through various methodologies. The ability of solar events to induce disturbances in both the ionosphere and the geomagnetic field is...

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Bibliographic Details
Published inRemote sensing (Basel, Switzerland) Vol. 15; no. 18; p. 4626
Main Authors López-Urias, Charbeth, Vazquez-Becerra, G. Esteban, Nayak, Karan, López-Montes, Rebeca
Format Journal Article
LanguageEnglish
Published Basel MDPI AG 01.09.2023
Subjects
Algorithms
Analysis
Approximation
Atmosphere, Upper
Composition
Data analysis
Geomagnetic field
Global positioning systems
GNSS
GPS
Ionosphere
Ionospheric disturbances
Navigation systems
Propagation
Radiation
Receivers & amplifiers
Remote sensing
Satellite communications
Sensors
Signal processing
Solar activity
solar flare
Solar flares
Structure
Sun
Total Electron Content
Wavelet analysis
Wavelet transforms
wavelets
Mexico
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Summary:The influence of solar activity on the ionosphere, a critical area of investigation due to its relevance to the Sun–Earth relationship, has been extensively examined through various methodologies. The ability of solar events to induce disturbances in both the ionosphere and the geomagnetic field is widely acknowledged. This specific study focused on sporadic incidents resulting from X-class solar flares that occurred between 2021 and 2022. Utilizing a methodology that involved analyzing data at 5Hz intervals using wavelet algorithms, the data from the GNSS stations of the National Autonomous University of Mexico (UNAM) were investigated. The primary emphasis was on deducing the Total Electron Content (TEC) within the ionosphere. Subsequently, this parameter for each satellite during instances of solar flares was analyzed. The approach uncovered disruptions in the ionosphere triggered by solar flares, even in cases where events transpired at the periphery of the solar disk and were of magnitudes smaller than X2.
ISSN:2072-4292
2072-4292
DOI:10.3390/rs15184626