Probing of medium-scale traveling ionospheric disturbances using HF-induced scatter targets

被引:8
|
作者
Blagoveshchenskaya, N. R. [1 ]
Borisova, T. D.
Kornienko, V. A.
Moskvin, I. V.
Rietveld, M. T.
Frolov, V. L.
Uryadov, V. P.
Kagan, L. M.
Yampolski, Yu. M.
Galushko, V. L.
Koloskov, A. V.
Kasheev, S. B.
Zalizovski, A. V.
Vertogradov, G. G.
Vertogradov, V. G.
Kelley, M. C.
机构
[1] Arctic & Antarctic Res Inst, St Petersburg 199226, Russia
[2] EISCAT Sci Assoc, Ramfjordbotn, Norway
[3] Radiophys Res Inst, Nizhnii Novgorod, Russia
[4] Univ Western Ontario, London, ON N6A 3K7, Canada
[5] NAS, Inst Radioastron, Kharkov, Ukraine
[6] Rostov Don State Univ, Rostov Na Donu, Russia
[7] Cornell Univ, Ithaca, NY USA
关键词
ionosphere; ionosphere : active experiments; ionospheric disturbances; radio science; nonlinear phenomena;
D O I
10.5194/angeo-24-2333-2006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Experimental results from the Tromso and Sura heating experiments at high and mid-latitudes are examined. It is shown that the combination of HF-induced target and bi-static HF Doppler radio scatter observations is a profitable method for probing medium-scale traveling ionospheric disturbances (TIDs) at high and mid-latitudes. HF ionospheric modification experiments provide a way of producing the, HF-induced scatter target in a controlled manner at altitudes where the sensitivity to TIDs is highest. Bi-static HF Doppler radio scatter observations were carried out on the London-Tromso-St. Petersburg path in the course of a Tromso heating experiment on 16 November 2004 when the pump wave was reflected from an auroral Es-layer. During Sura heating experiments on 19 and 20 August 2004, when the HF pump wave was reflected from the F2 ionospheric layer, multi-position bi-static HF Doppler radio scatter observations were simultaneously performed at three reception points including St. Petersburg, Kharkov, and Rostov-on-Don. Ray tracing and Doppler shift simulations were made for all experiments. A computational technique has been developed allowing the reconstruction of the TID phase velocities from multi-position bi-static HF Doppler scatters. Parameters of medium-scale TIDs were found. In all experiments they were observed in the evening and pre-midnight hours. TIDs in the auroral E-region with periods of about 23 min were traveling southward at speeds of 210 m/s. TIDs in the mid-latitudinal F-region with periods from 20 to 45 min travelled at speeds between 40 and 150 m/s. During quiet magnetic conditions the waves were traveling in the north-cast direction. In disturbed conditions the waves were moving in the south-west direction with higher speeds as compared with quiet conditions. Possible sources for the atmospheric gravity waves at middle and high latitudes are discussed.
引用
收藏
页码:2333 / 2345
页数:13
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