Geoscience Reference
In-Depth Information
Fig. 15.4.
Trajectory of satellite AUREOL-3 during the MASSA experiment: 1)
location of the satellite at time of the explosion, 2) point where the satellite trajec-
tory intersects the explosion's field tube, and 3) location of the satellite above the
shot size
The Alfven Pulse
Measurements by an airborne magnetometer showed a significant magnetic
variation at
t
= 298 s at a distance of about 700 km from the explosion's field
tube, and
L
=1
.
31 (see Fig. 15.6) ([5], [6]). Characteristic features of this
Fig. 15.5.
Theelectricalfieldforaseriesofbandfiltersintherange10to200
Hz at the intersection of the explosion's magnetic field tube (left panel. Arbitrary
units). The dashes are the background of the EZ-component (approximately along
the magnetic field) and the EH-component (across the field).
EH
and
EZ
at fre-
quencies 15 and 4.5 kHz along the orbit is shown in the right panel. The background
noise level is shown by the dashed lines
Search WWH ::
Custom Search