UNUSUAL WAVE PHENOMENA NEAR
INTERPLANETARY SHOCKS AT HIGH-LATITUDES
THEJAPPA G
WENTZEL DG
MACDOWALL RJ
STONE RG
GEOPHYSICAL RESEARCH LETTERS
v.22, n.23, DEC 1, 95, p.3421-3424
We report on several interplanetary shocks that are
unusual because waves at about 10 Hz
are highly electrostatic in the upstream region yet highly
electromagnetic in the downstream
region. These shocks, detected by the Unified Radio and
Plasma Wave Experiment (URAP)
on Ulysses are supercritical reverse shocks, which
occurred predominantly at high
heliographic latitudes. The level of wave activity is
observed to be independent of the angle
between the magnetic field and the shock normal, the Mach
number, and the change in the
ratio of ion t hermal pressure to magnetic pressure from
upstream to downstream regions.
Since the energy in the upstream electrostatic waves is
small compared to the downstream
electromagnetic waves, mode conversion from electrostatic
to electromagnetic at the shock is
not a viable mechanism. The upstream and downstream waves
are likely to be generated by
separate mechanisms, with lower hybrid waves being the
most probable candidates for the
upstream waves and electromagnetic l ower hybrid or
whistlers for the downstream waves.