2022
DOI: 10.1016/j.asr.2022.02.031
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Statistical study on the characterization of phase and amplitude scintillation events in the high-latitude region during 2014–2020 based on ISMR

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Cited by 4 publications
(2 citation statements)
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“…Furthermore, to reduce the impact of multipath, the 20‐degree elevation mask is adopted, which was utilized by previous scintillation investigations (e.g., Béniguel, 2019; Salles et al., 2021; Veettil et al., 2020). Meanwhile, to avoid other nonscintillation‐related disturbances on BDS signals, 0.2 is selected as the threshold of the amplitude scintillation index S 4 indicating the occurrence of ionospheric scintillation at the given epoch (Luo et al., 2020; Muella et al., 2009, 2014; Pasumarthi et al., 2020; Zhao et al., 2022), characterized by the standard deviation of I /< I >, where I is the received signal intensity (power) and < > represents temporal averaging, typically during a 60‐s interval, assuming a sampling frequency of 50 Hz (Luo et al., 2020; Moraes et al., 2019; Song et al., 2022; Sousasantos et al., 2018), to indicate the occurrence of ionospheric scintillation. Ionospheric scintillation events were further classified as weak (0.2 ≤ S 4 < 0.4), moderate (0.4 ≤ S 4 < 0.6), and intense ( S 4 ≥ 0.6) (Humphreys et al., 2010; Vilà‐Valls et al., 2020).…”
Section: Description Of Measurements and Data Processingmentioning
confidence: 99%
“…Furthermore, to reduce the impact of multipath, the 20‐degree elevation mask is adopted, which was utilized by previous scintillation investigations (e.g., Béniguel, 2019; Salles et al., 2021; Veettil et al., 2020). Meanwhile, to avoid other nonscintillation‐related disturbances on BDS signals, 0.2 is selected as the threshold of the amplitude scintillation index S 4 indicating the occurrence of ionospheric scintillation at the given epoch (Luo et al., 2020; Muella et al., 2009, 2014; Pasumarthi et al., 2020; Zhao et al., 2022), characterized by the standard deviation of I /< I >, where I is the received signal intensity (power) and < > represents temporal averaging, typically during a 60‐s interval, assuming a sampling frequency of 50 Hz (Luo et al., 2020; Moraes et al., 2019; Song et al., 2022; Sousasantos et al., 2018), to indicate the occurrence of ionospheric scintillation. Ionospheric scintillation events were further classified as weak (0.2 ≤ S 4 < 0.4), moderate (0.4 ≤ S 4 < 0.6), and intense ( S 4 ≥ 0.6) (Humphreys et al., 2010; Vilà‐Valls et al., 2020).…”
Section: Description Of Measurements and Data Processingmentioning
confidence: 99%
“…One of the main equipment on monitoring scintillations is the ionospheric scintillation monitoring receiver (ISMR), which can provide two types of indices: the amplitude scintillation index (S4 ${S}_{4}$) and the phase scintillation index (σϕ ${\sigma }_{\phi }$). Due to the differences in the generation mechanism of ionospheric scintillation in the low latitude and the polar regions (Luan et al., 2015; Mitchell et al., 2005), amplitude scintillations often occur in the low latitude region, while phase scintillations dominate in the polar region (Zhao, Li, Wang, et al., 2022). To reflect the variation information of the scintillation in the Arctic region, which is the interest area of this research, the phase scintillation index will be extensively studied in this paper.…”
Section: Introductionmentioning
confidence: 99%