Probing of medium-scale traveling ionospheric disturbances using HF-induced scatter targetsN. F. Blagoveshchenskaya1, T. D. Borisova1, V. A. Kornienko1, I. V. Moskvin1, M. T. Rietveld2, V. L. Frolov3, V. P. Uryadov3, L. M. Kagan4, Yu. M. Yampolski5, V. L. Galushko5, A. V. Koloskov5, S. B. Kasheev5, A. V. Zalizovski5, G. G. Vertogradov6, V. G. Vertogradov6, and M. C. Kelley71Arctic and Antarctic Research Institute, St. Petersburg, Russia
2EISCAT Scientific Association, Ramfjordbotn, Norway
3Radiophysical Research Institute, Nizhny Novgorod, Russia
4University of Western Ontario, London, ON, Canada
5Institute of Radio Astronomy NAS, Kharkov, Ukraine
6Rostov-on-Don State University, Rostov-on-Don, Russia
7Cornell University, Ithaca NY, USA
Abstract. Experimental results from the Tromsø 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-Tromsø-St. Petersburg path in the course of a Tromsø
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-east
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.
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Citation: Blagoveshchenskaya, N. F., 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., and Kelley, M. C.: Probing of medium-scale traveling ionospheric disturbances using HF-induced scatter targets, Ann. Geophys., 24, 2333-2345, 2006. Bibtex EndNote Reference Manager