First results on low-latitude E and F region irregularities obtained using the Gadanki Ionospheric

被引:48
|
作者
Patra, A. K. [1 ]
Srinivasulu, P. [1 ]
Chaitanya, P. Pavan [1 ]
Rao, M. Durga [1 ]
Jayaraman, A. [1 ]
机构
[1] Natl Atmospher Res Lab, Gadanki, India
关键词
EQUATORIAL SPREAD-F; FIELD-ALIGNED IRREGULARITIES; VHF RADAR OBSERVATIONS; ATMOSPHERE RADAR; STATISTICAL CHARACTERISTICS; NUMERICAL SIMULATIONS; PLASMA DEPLETIONS; KILOMETER-SCALE; ELECTRIC-FIELD; 150-KM ECHOES;
D O I
10.1002/2014JA020604
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A 30 MHz radar has recently been established at Gadanki (13.5 degrees N, 79.2 degrees E; 6.5 degrees N magnetic latitude) to make unattended observations of the ionospheric field-aligned irregularities (FAI). This radar, called the Gadanki Ionospheric Radar Interferometer (GIRI), has been designed to have scanning capability of 100 degrees in the east-west plane perpendicular to Earth's magnetic field and interferometry/imaging system to study drifts and spatial distribution of plasma irregularities at both large and small scales. In this paper, we present the first results on the E and F region FAI made using the scanning capability of the GIRI. Daytime observations of E region FAI show type 2 echoes with velocities predominantly upward northward (downward-southward) at altitudes >100 km(<100km) and westward (eastward) in the forenoon (afternoon) with signature of tidal wind field. F region irregularities show bottom-type, bottomside and plume structures with close resemblance to those observed over the magnetic equator. Observations made with the east-west scanning capability have been used to study the origin, evolution, and drift of the FAI for the first time from Gadanki. Eastward drifts are estimated to be 90-210 m s(-1) during 20-24 LT. Upward velocity as large as 500 m s(-1) has been observed in the initial phase of the plume structures. Intriguingly, downward velocity as large as 60 m s(-1) has also been observed in the plumes, displaying descending pattern, observed in the early evening hours. These results are presented and discussed in the light of current understanding of low-latitude plasma irregularities, and future prospects of GIRI are outlined.
引用
收藏
页码:10,276 / 10,293
页数:18
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