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Fig. 5.8
Same as in Figs.
5.6
and
5.7
, but for other temporal sampling. Taken from Surkov et al.
(
2006
)
Fig. 5.9
Nighttime power
spectra of 1-h temporal
sequence (from 2;100 till
2;200 LT) observed at
Karimshino station on 13
September 2000. Taken from
Surkov et al. (
2006
)
is estimated as 2 s, which is close to the signal duration. As is seen from Fig.
5.7
(the
second line panels, D-component), the signal occasionally contains three distinct
impulses at least. This implies a possibility for multiple wave reflections from the
IAR upper and lower boundaries.
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