2016
DOI: 10.1080/19475705.2016.1246483
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Statistical discrimination of global post-seismic ionosphere effects under geomagnetic quiet and storm conditions

Abstract: The retrospective statistical analysis of total electron content (TEC) is carried out using global ionospheric maps (GIM) for 1999-2015. TEC anomalies are analysed for 2670 earthquakes (EQ) from M6.0 to M10.0 classified into 2205 'non-storm' EQs and 465 'storm' EQs during geomagnetic storms. The geomagnetic storms are specified by relevant thresholds of geomagnetic indices AE, aa, ap, ap(t) and Dst. Using slidingwindow statistical analysis, moving daily-hourly TEC median m for 15 preceding days with estimated … Show more

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Cited by 19 publications
(5 citation statements)
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“…In terms of the geomagnetic condition, the mean Kp and mean Dst were 2.5 and −13.0 nT, respectively. These two values are below the thresholds for active geomagnetic conditions, which are larger than 3 for Kp index (Mungufeni et al, 2016) and smaller than −20 nT for Dst index (Gulyaeva & Arikan, 2017). In terms of solar condition, the F10.7 index varied smoothly with a mean of 84.3 sfu, which is also below the threshold of active solar conditions, that is, 150 sfu (Tapping, 2013).…”
Section: Geomagnetic and Solar Conditionsmentioning
confidence: 98%
“…In terms of the geomagnetic condition, the mean Kp and mean Dst were 2.5 and −13.0 nT, respectively. These two values are below the thresholds for active geomagnetic conditions, which are larger than 3 for Kp index (Mungufeni et al, 2016) and smaller than −20 nT for Dst index (Gulyaeva & Arikan, 2017). In terms of solar condition, the F10.7 index varied smoothly with a mean of 84.3 sfu, which is also below the threshold of active solar conditions, that is, 150 sfu (Tapping, 2013).…”
Section: Geomagnetic and Solar Conditionsmentioning
confidence: 98%
“…Firstly, the variations of Kp, Dst, and F10.7 (Rostoker 1972) indices during the Usagi were studied because the strong geomagnetic and solar activities can also induce the ionospheric disturbance (Moeketsi et al 2007;Brunini and Azpilicueta 2010;Guo et al 2017). For a quiet geomagnetic condition, the Kp index should be smaller than 3 (Mungufeni et al 2016), and the Dst index should be larger than − 20 nT (Gulyaeva and Arikan 2017). For a relatively quiet solar condition, the F10.7 index should be smaller than 150 sfu (Tapping 2013).…”
Section: Ionospheric Conditionmentioning
confidence: 99%
“…State of the ionosphere changes due to geomagnetic activity (Mandea & Korte, 2010). It is important to distinguish between extreme behavior in ionospheric state due to geomagnetic storms and seismic activity (Gulyaeva & Arikan, 2017; Gulyaeva et al, 2016, 2017a). Ionosphere‐based parameters are widely used to assess the state of the ionosphere in terms of geomagnetic activities and geomagnetic storms.…”
Section: Data Used By the Proposed Eq‐pd Techniquementioning
confidence: 99%