Probing of medium-scale traveling ionospheric disturbances using HF-induced scatter targets
Permanent lenke
https://hdl.handle.net/10037/2418Dato
2006-09-20Type
Journal articleTidsskriftartikkel
Peer reviewed
Forfatter
Blagoveshchenskaya, N. F.; Rietveld, Michael T.; Borisova, T. D.; Kornienko, V. A.; Moskvin, I. V.; 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.Sammendrag
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, multiposition
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.
Forlag
European Geosciences Union (EGU)Sitering
Annales Geophysicae, 24, 2333–2345, 2006Metadata
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