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2018
DOI: 10.1016/j.jastp.2017.10.009
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Nighttime lower ionosphere height estimation from the VLF modal interference distance

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Cited by 9 publications
(8 citation statements)
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“…The ionosphere height arose to about 100 km, 5-10 km higher than its surrounding areas from June to August, at latitudes of about ±30 • and longitudes between 90 • and 150 • . Samanes [38] studied its nighttime features at the equatorial region for the western longitudes by using data from the DEMETER satellite and ground VLF receivers, and they found typical seasonal characteristics with lower values in winter time compared to summer time. The effective height in the Indonesia seismic area, as derived in our study, should increase or maintain a relatively high value during July and August, according to [37] and [38].…”
Section: Discussionmentioning
confidence: 99%
“…The ionosphere height arose to about 100 km, 5-10 km higher than its surrounding areas from June to August, at latitudes of about ±30 • and longitudes between 90 • and 150 • . Samanes [38] studied its nighttime features at the equatorial region for the western longitudes by using data from the DEMETER satellite and ground VLF receivers, and they found typical seasonal characteristics with lower values in winter time compared to summer time. The effective height in the Indonesia seismic area, as derived in our study, should increase or maintain a relatively high value during July and August, according to [37] and [38].…”
Section: Discussionmentioning
confidence: 99%
“…However, the findings of Sharma et al () did agree with Silber et al () that the SAO is the strongest oscillation detected in midlatitude nighttime VLF measurements. Using the Lomb‐Scargle method, periodicities related to the AO, SAO, and quasi biennial oscillation were reported by Samanes et al (). They analyzed the derived nighttime reflection height using signals that propagated in low‐latitude regions.…”
Section: Introductionmentioning
confidence: 96%
“…Periodic variations of solar (Demirkol et al, ; Thomson & Clilverd, ) and terrestrial (Samanes et al, ) origin affect recorded VLF signals over long‐ or short‐time scales. Many studies show long‐term periodic variations of solar origin, such as the 11‐year solar cycle, in the lower ionosphere (e.g., Macotela et al, ; Thomson & Clilverd, ).…”
Section: Introductionmentioning
confidence: 99%
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