2017
DOI: 10.1002/2016ja023647
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First observation of presunset ionospheric F region bottom‐type scattering layer

Abstract: The bottom‐type irregularity scattering layer (BSL) that can appear in the ionospheric F region bottomside has been observed generally after sunset, serving as a possible telltale of equatorial spread F (ESF). Using simultaneous multibeam radar measurements over two low‐latitude stations, Sanya (18.3°N, 109.6°E; dip latitude 13°N) and Fuke (19.3°N, 109.1°E; dip latitude 14°N) in China, we report, for the first time, a thin BSL that initially occurred at presunset (~1720 LT), much earlier than the occurrence of… Show more

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Cited by 23 publications
(49 citation statements)
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“…The center beam is pointed to geographic north with the zenith angle of 28.2°. The 3 dB (half power full beam) beam width is 21° in the north‐south direction, and all the beams can satisfy the perpendicular condition to geomagnetic field lines at both ionospheric E and F regions (e.g., Li et al, ). Figure a shows the radar beam directions (blue lines labeled 1 to 7 from east to west) in the geographic longitude‐latitude plane.…”
Section: Instruments and Datamentioning
confidence: 99%
“…The center beam is pointed to geographic north with the zenith angle of 28.2°. The 3 dB (half power full beam) beam width is 21° in the north‐south direction, and all the beams can satisfy the perpendicular condition to geomagnetic field lines at both ionospheric E and F regions (e.g., Li et al, ). Figure a shows the radar beam directions (blue lines labeled 1 to 7 from east to west) in the geographic longitude‐latitude plane.…”
Section: Instruments and Datamentioning
confidence: 99%
“…The radar has a wide 3‐dB beam width (36° in the north‐south direction) that satisfies the perpendicular condition to the magnetic field lines from E to F regions and can receive the coherent echoes arising from field‐aligned irregularities in these regions. For additional details about the radar parameters please see Li et al (, ). The ionosonde (DPS‐4D) colocated at Sanya is employed to get the ionospheric background condition.…”
Section: Datamentioning
confidence: 99%
“…Many sources such as weather storm, earthquake, and solar storm can launch gravity waves/acoustic waves in the atmosphere. The waves propagate through the thermosphere, generating plasma density disturbances with varying periods of minutes to hours (e.g., Lay et al, ; Negrea et al, ; Negrea & Zabotin, ; Yue et al, ) and triggering plasma thin layer and/or plume‐type irregularities in the ionosphere (e.g., Abdu et al, ; Fritts et al, ; Li et al, ). With regard to the wavelength/period, ionospheric disturbances can be classified into three types: large, middle, and small scales.…”
Section: Introductionmentioning
confidence: 99%