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The most intense irregularities in both hemispheres were observed after 16 UT on 22 June.
Moreover, the highly intense irregularities lead to a performance degradation of the European Geostationary Navigation Overlay Service EGNOSS).
A very specific signature of the irregularity pattern is clearly recognized, where intense irregularities are oriented in the day night direction across the polar cap.
The most intense irregularities in the high and mid-latitudes were found to occur at 18-22 UT on 22 June, which were associated with a new period of the increased auroral activity with two peaks of the AE index of ~2180 and ~2700 nT, observed at 18 49 and 20 10 UT, respectively.
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The most intense ionospheric irregularities were found within 60 70° MLAT during ~20 09 MLT and one noontime peak at ~11 13 MLT.
During the main phase of this storm, the zone of the intense ionospheric irregularities occurrence moved equatorward (Fig. 3).
Over the Northern Hemisphere, the most intense ionospheric irregularities are found within 60° 70° MLAT during ~20 09 MLT, with one noontime peak observed at ~1100 1300 MLT.
During disturbance day of 17 March, the intense ionospheric irregularities at altitude of about 500 km in comparison with the quiet-day ones were observed.
The ROTI values marked by orange and red colors (ROTI >0.8 1.0 TECU/min) correspond to the occurrence of the intense ionospheric irregularities in this sector.
However, the LEO ROTI maps do not show intense ionospheric irregularities near and within the auroral region at that time, with an equatorward border around 60° MLAT.
Relatively good agreement between the auroral model boundaries and intense GPS irregularities location is found in night-time sector of 21 03 MLT.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com