Geoscience Reference
In-Depth Information
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.
Search WWH ::




Custom Search