Generation of auroral kilometric radiation by electron horseshoe distributions

High time resolution of rocket and satellite electron distribution function s within the source region of auroral kilometric radiation display a charac teristic crescent shaped or horseshoe distribution. Such distribution funct ions are created by a field aligned electron beam moving into an increasing magnetic field, conservation of the first adiabatic invariant causes an in crease of their pitch angle. This produces a broad region on the distributi on function where partial derivative f(e)/partial derivative v(perpendicula r to)> 0, and is a possible source of free energy leading to radio wave emi ssion by the cyclotron maser instability, which is more efficient than the conventional loss-cone maser instability. The stability of these electron h orseshoe distribution functions is examined for right-hand extraordinary mo de (R-X mode) radiation close to the electron cyclotron frequency propagati ng perpendicular to the magnetic field. (C) 2000 American Institute of Phys ics. [S1070-664X(00)00907-1].