2019
DOI: 10.1007/s11600-019-00319-w
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Assessment of signal processing methods for geomagnetic precursor of the 2012 M6.9 Visayas, Philippines earthquake

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Cited by 26 publications
(16 citation statements)
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“…In theory, the amplitude of P Z/G would increase anomalously due to the direct lithospheric emission a few weeks to several days before an earthquake. This observation was reported by prior studies [14][15][16].…”
Section: Introductionsupporting
confidence: 86%
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“…In theory, the amplitude of P Z/G would increase anomalously due to the direct lithospheric emission a few weeks to several days before an earthquake. This observation was reported by prior studies [14][15][16].…”
Section: Introductionsupporting
confidence: 86%
“…Similarly, nighttime period, ∆T, also differed across studies; thus, five different periods (∆T = 22-02, 23-03, 00-04, 01-05 and 02-06 LT) were examined for each earthquake to identify the least geomagnetically disturbed period at which precursors appeared. An anomaly is identified when the P Z/G value of a particular day exceeds the mean plus two times the standard deviation (µ + 2σ) of the entire period of observation [15]. If the anomaly appeared during an undisturbed period, then the anomaly was assumed to be a possible precursor.…”
Section: Precusor Detectionmentioning
confidence: 99%
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“…The method to study the earthquake is polarization ratio. The polarization ratio analysis method has successfully detected an anomaly preceding the main earthquake (Yusof et al, 2019). The H-component or Horizontal intensity is suitable to study the geomagnetic storm.…”
Section: Period Of Studymentioning
confidence: 99%
“…However, the ULF emission that can be assigned as electromagnetic anomalies has sometimes been problematic because not only is the intensity very weak (around 1nT) but it is usually difficult to understand as well due to the intense natural background of the geomagnetic field [8]. To distinguish between the emission and the background, polarization analysis has been applied to separate the vertical component of the geomagnetic field from the horizontal component [9,10]. The Comparative Polarization signal for the H and Z components separates the ULF emission of solar wind, magnetosphere, ionosphere, or lithosphere and is derived from seismic origins [11].…”
Section: Introductionmentioning
confidence: 99%