28 Nov 2001
Einar Mjølhus "HF-driven Langmuir turbulence in the ionosphere"."HF" stands for "High Frequency", in this case High
Frequency radio wave, "Langmuir turbulence" stands for a plasma
turbulence involving Langmuir modes (and what is a Langmuir mode? Correct, a
certain wave mode in a plasma.).
If we send an electromagnetic wave into a plasma, it can start processes that
increase the fraction of its energy that is absorbed in the plasma, so that this
fraction increases with the intensity of the electromagnetic wave. Many of these
processes have the character of a parametric instability. It is the saturated
stage of one such process that is referred to above as "Langmuir
turbulence". The plasma of the ionosphere ~200km above us has turned out to
be a well suited laboratory for the study of this process, with the
driving "HF" radio wave transmitted by an antenna system (the
"Heating" facility) at Ramfjordmoen 25km outside Tromsø, and with the
EISCAT radars as diagnostics.
In 1972, V. E. Zakharov published a model for Langmuir turbulence which we today
call "the Zakharov model". An outcome of that model is
"collapse" - that a finite amount of energy contracts to a point in
finite time. One issue I shall discuss, is whether manifestations of such
phenomena will be/has been observable by the experimental set-up described
above.
I thought to use two seminars for this. It will be about physics, maybe with a
minor attention to numerical methods and some to the modelling. I intend to keep
everything at a simple qualitative/untechnical level, including a five minutes'
crash course in plasma physics.