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First results on low-latitude E and F region irregularities obtained using the Gadanki Ionospheric
被引:46
|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.
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页码:10,276 / 10,293
页数:18
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