INTERNATIONAL JOURNAL OF GEOMAGNETISM AND AERONOMY VOL. 5, GI3006, doi:10.1029/2005GI000103, 2005
3. Features of the Magnetic Storm
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Figure 1
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Figure 2
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Figure 3
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Figure 4
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Figure 5
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[7] Let us consider the character of the studied magnetic storm on
14-17 May 1997. From different sources of geophysical data
available on through the Internet (SPIDR, SDAWeb, IDCE, Kyoto
WDC C2, Sodankyla, etc.) one can find that the onset of the storm
took place at 1600 UT on 14 May 1997 and it ended in the evening
of 17 May 1997. So, by analyzing data of the IMP 8 satellite, a
sharp increase of solar wind velocity (flow speed) from
300 km s-1 to 500 km s-1 occurs from 1600 UT (14 May
1997) till 0600 UT (15 May 1997), flux of protons with energy
> 1 MeV for this period increases 5 times, and the average field
magnitude of the IMF increases also 5 times (from 5 up to 25 nT).
The Kp index grows from 1 to 7 for the considered period and the
Dst index has a maximum at 1200 UT on 15 May 1997. In the
evening of 17 May 1997 all mentioned parameters are near to the
initial data before 1600 UT on 14 May 1997 again. One can see in
Figures 1,
2,
3,
4, and
5
the corresponding variations of the parameters
AE,
Bz component and riometer absorption. For example, at 1700 UT
on 14 May 1997 the
Bz value (see Figure 1f) reaches the minimum
negative value, the maximum of the
AE index is reached at
1800 UT. Further,
Bz minima are at 2000 UT on 14 May 1997;
0630 UT on 15 May 1997; 1100 UT on 15 May 1997; 1400 UT on 16 May
1997; 2300 UT on 16 May 1997 and approximately one hour later
there are the
AE maxima at: 2100 UT on 14 May 1997; 0730 UT on
15 May 1997; 1200 UT on 15 May 1997; 1500 UT on 16 May 1997 and
2400 UT on 16 May 1997. Such behavior of the
Bz and
AE indexes is classical [Rostoker et al., 1980].
From 0100 UT on 17 May 1997
Bz data are absent. Sharp growth of
riometer absorption
A (Figure 1d) occurs at 1700 UT on 14 May
1997. Further, absorption has moderate values (about
A > 1 dB)
till evening hours on 17 May 1997. The period from 0000 till 1600
UT for 14 May 1997 and the full day on 18 May 1997 (Figure 5)
could be classified as slightly disturbed or nearly quiet because
the
AE indexes do not exceed 150-200 nT, values of the
Kp indexes do not exceed 2 and the absorption
A < 0.5 dB.
Citation: Blagoveshchensky, D. V., S. V. Nozdrachev, M. A. Sergeeva, and P. A. Sinyansky (2005), Magnetic storm effects on a HF transauroral radio path, Int. J. Geomagn. Aeron., 5, GI3006, doi:10.1029/2005GI000103.
Copyright 2005 by the American Geophysical Union
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