Fifth LOIS Workshop, November 23-25, 2003
LOIS Space Centre, Växjö, Sweden
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Accelerated electrons and UHF SEE, airglow and additional ionization in
ionospheric modifications
(1) S. M. Grach, (2) E. N. Sergeev, (2) V. M. Fridman,(3) A. M. Nasyrov
(1) State University of Nizhny Novgorod
(2) Radiophysical Research Institute
(3) Kazan State University
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Abstract
Results of experimental studies of three different phenomena related to
appearance of energetic (accelerated) electrons during ionospheric
modifications by powerful HF radio waves are discussed.
First, the HF pumping of the ionospheric F-region at the frequencies
4.5--7 MHz causes the enhancement of the electromagnetic emission from
the pumped volume of the ionosphere at the frequencies f~600 MHz by
0.3$--1.3 K. The emission is excited at the altitudes 195--220 km above
the Sura facility. The characteristic times of the UHF SEE development
and decay were found to be of order of few tens of seconds. The
emission is tentatively attributed to an excitation of high Rydberg
states of the neutral particles by the accelerated electrons, but this
requires further experimental and theoretical study.
Second, the results of correlated study of the pump induced optical
emission in the green line of atomic oxygen (conditioned by accelerated
electrons) and the HF SEE are presented for special diagnostic schedule
of the pumping are presented. It our experiments the airglow was
observed just after transition of the pump wave from the continuous
radiation to short pulse radiation. This corresponds to the initial
stage of the decay of so-called striations, which is confirmed by HF SEE
measurements.
Third, accelerated electrons cause an additional ionization of the
ionospheric plasma. The additional ionization is studied by
multifrequency Doppler sounding of the ionosphere modified volume. In
our experiments, a dependence of the additional ionization efficiency on
the relation between the pump frequency and harmonics of the electron
cyclotron frequency was investigated for the 4th, 5th and 6th harmonics.
The work is supported by RFBR grant no. 03-02-16309.
The presentation (PDF)
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