Priming the Electron Distribution
A heating or "priming" of the electron distribution
beyond the
heliopause is an important component of our group's theory for the outer
heliospheric
radio emission. The process begins when high speed neutral particles,
formed by
collisions between solar wind protons and interstellar medium neutrals
in the inner
heliosheath, cross the heliopause and enter the outer heliosheath and
interstellar
medium. These high speed particles collide with interstellar protons
and undergo
charge exchange for a second time giving rise to high speed protons
which are then
"picked up" by the local magnetic field and begin to gyrate about it (hence
they are
called "pick-up ions"). The pick-up ions form a ring-beam distribution in
velocity
space with the ring perpendicular to the magnetic field, which can generate
lower-hybrid waves. These waves in turn can resonantly accelerate electrons,
forming
a non-thermal tail on the electron distribution. This process is known
as lower-hybrid
drive (LHD).
Recent work in this area predicts that the inclusion
of the LHD tail may increase the
power of shock driven radiation by four orders of magnitude. As
well as conducting
research into the implications of electron distibution priming, our
group is also
working to improve the current model of the LHD process.
Publications
- I.H. Cairns and G.P. Zank, Turn on of the 2-3 kHz radio emission Beyond the
heliopause, Geophys. Res. Lett., 29(7), 47, 2002.
- J.J. Mitchell, I.H. Cairns and P.A. Robinson, Theory for the 2-3 kHz radiation from
the outer heliosphere, J. Geophys. Res., 109, A06180, 2004.
- J.J. Mitchell, I.H. Cairns, H.-R. Müller,
G.P. Zank, Timing of the 2-3 kHz radio
emission within the solar cycle, Geophys. Res. Lett., in press, 2005.
Other outer heliosphere projects
- The propagation of radiation using ray tracing
- Draping of the magnetic field over the heliopause
- Radio emission in the outer heliosphere
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