The conditions for different IMF clock angles
are better
discussed together with the IMF cone angle
.For instance, when
is very small, the magnetic field
is basically along the Sun-Earth line regardless of the value of
.Conversely,
becomes important in determining the
IMF orientation when
is large.
Previously, it was shown in Figure 6 that low
angles
are favorable for the occurrence of the P4 (16-32 mHz)
and P5 (32-64 mHz) events.
This trend is also clearly found in Figure 7.
In contrast to the P2 events, the P5 (32-64 mHz)
events occur predominantly
when
and when the IMF is northward
(
).
Moving toward lower frequencies, the waves tend to occur more
under high
conditions.
The conditions for the P3 and P4 events
seem to be mixtures of the two extremes.
It should be noted here that the comparison between the results
of two neighboring frequency bands needs to be made with some caution.
If a wave event has the peak frequency located at the boundary between
two frequency bands, it will be counted as an event in only one of the
two bands because of the nature of the selection criterion.
As a result, the occurrence patterns for the two neighboring
frequency bands may look complementary to some degree.
For example, P4 has a high occurrence rate when
and
,but the occurrence rate of P5 shows a deficit at the same
IMF orientation (Figure 7).
However, this effect should not be significant since the number of
events for any frequency band is less than 30% of the total
entries of the database.
In addition, for the two frequency bands that are
not adjacent to each other, their events are selected
independently.
For example, the difference between the occurrence patterns of P2
and P5 reflects reality rather than an artifact of
the selection criterion.
| Figure 7. Normalized occurrence rates for |