The dependences of the nighttime low‐latitude F‐region 3.2‐m‐scale field‐aligned irregularities (FAIs) occurrence and vertical drift on solar activity, season, and magnetic activity during 2014–2017 are studied by using the coherent scatter radar located at Fuke (19.5°N, 109.1°E) and a nearby Digisonde at Sanya (18.4°N, 109.6°E), Hainan Island, China. The postsunset FAIs occurrence and vertical drift are closely related and modulated by the solar activity, especially for equinox. Utilizing the day‐to‐day comparison analysis, the threshold of the peak Vz for the definitive postsunset FAIs generation during equinox was ∼30 m/s. The postmidnight FAIs occurrence in June solstice did not increase with the decreasing solar activity and is differe...
We used equatorial measurements from the ROCSAT-1 satellite to determine the seasonal and longitudin...
208-219In this paper a comparative study on equatorial F-region irregularities observed during the ...
A comparative study of the equatorial spread F occurrence was conducted at different longitudes duri...
In this paper, we present a study of the low‐latitude field‐aligned irregularities formation and evo...
Ionospheric plasma drift data in Hainan during the period of from Mar 2002 to Mar 2004 are analyzed ...
184-198A 47.5 MHz VHF radar with a peak power of 24 kW has been operated at Sanya (18°N, 109°E, dip...
The climatological characteristics of UHF-band scintillations over the low-latitude region of China ...
We use extensive incoherent scatter radar observations from the Jicamarca Radio Observatory to study...
For the first time, we develop a local time and day of year dependent climatological model in differ...
[1] We use extensive incoherent scatter radar observations made at the Jicamarca Radio Observatory b...
We use incoherent scatter radar measurements from the Jicamarca Observatory to study the variability...
Abstract In order to statistically investigate the relationship between the low-latitude coronal hol...
A study of the seasonal, solar, and magnetic activity dependence of the evening F region vertical pl...
We investigate the regularities of a change in Spread-F F probability during day-to-day, under varyi...
Abstract The east–west component of magnetic field variation (∆D-component) at Davao station (Philip...
We used equatorial measurements from the ROCSAT-1 satellite to determine the seasonal and longitudin...
208-219In this paper a comparative study on equatorial F-region irregularities observed during the ...
A comparative study of the equatorial spread F occurrence was conducted at different longitudes duri...
In this paper, we present a study of the low‐latitude field‐aligned irregularities formation and evo...
Ionospheric plasma drift data in Hainan during the period of from Mar 2002 to Mar 2004 are analyzed ...
184-198A 47.5 MHz VHF radar with a peak power of 24 kW has been operated at Sanya (18°N, 109°E, dip...
The climatological characteristics of UHF-band scintillations over the low-latitude region of China ...
We use extensive incoherent scatter radar observations from the Jicamarca Radio Observatory to study...
For the first time, we develop a local time and day of year dependent climatological model in differ...
[1] We use extensive incoherent scatter radar observations made at the Jicamarca Radio Observatory b...
We use incoherent scatter radar measurements from the Jicamarca Observatory to study the variability...
Abstract In order to statistically investigate the relationship between the low-latitude coronal hol...
A study of the seasonal, solar, and magnetic activity dependence of the evening F region vertical pl...
We investigate the regularities of a change in Spread-F F probability during day-to-day, under varyi...
Abstract The east–west component of magnetic field variation (∆D-component) at Davao station (Philip...
We used equatorial measurements from the ROCSAT-1 satellite to determine the seasonal and longitudin...
208-219In this paper a comparative study on equatorial F-region irregularities observed during the ...
A comparative study of the equatorial spread F occurrence was conducted at different longitudes duri...