[6] The experiment was carried out on 18-22 August 2003 from
1600 to 2000 LT (
[7] The effective emission power PG was 40 or 80 MW
depending on the working frequency
fp. To control the radio
wave condition at the Khabarovsk-SURA, Irkutsk-SURA, and
Inskip-SURA paths, the reception of LFM signals at the paths
Khabarovsk-Nizhny Novgorod ( j = 56.1oN,
l = 44.1oE),
Irkutsk-Nizhny Novgorod, and Inskip-Nizhny Novgorod was
organized. The LFM sounders in Irkutsk and Khabarovsk
operated the first and the second halves of each hour,
respectively. The emission of the LFM signals started at 0, 5,
10,... 55 min of each hour with the following parameters:
starting frequency 4 MHz, end frequency 30 MHz, and rate of
the frequency returning 100 kHz s
-1. On 20 August 2003 when
the LFM sounders in Irkutsk and Khabarovsk did not operate,
the emission of the LFM sounder from England (Inskip) was
received. This sounder operated in the 5-min regime starting
from the second minute of each hour with the following
parameters: starting frequency 4.2 MHz, end frequency 30 MHz,
and rate of the frequency returning 100 kHz s
-1. The LFM signals
in the Rostov-on-Don reception point were received by the oblique
V antenna oriented to the SURA heating facility. The same
antenna was used to receive the etalon signals of the RVM
station at a frequency of 9996 kHz. The RVM transmitter
operated in a regime of continuous emission of the carrier from
0 to 8 s and from 30 to 38 s of every hour. During the operation
of the SURA facility the RVM transmitter was used as a
Doppler HF radar at the RVM sounding path Moscow
( j =55.3 o N,
l = 38.7oE) to
SURA-Rostov on Don for diagnostics of
artificial small-scale magnetically oriented irregularities. In the
Nizhny Novgorod reception point the LFM signals were
received using the vertical collapsible whip. The geometry of
the experiment is shown in Figure 1.
Citation: 2004), Ionospheric effects of the magnetic storm on 18--22 August 2003 according to the data of HF sounding of the artificial ionospheric turbulence, Int. J. Geomagn. Aeron., 5, GI1007, doi:10.1029/2003GI000059.
Figure 1
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