Fullekrug, M.3; Roussel-Dupre, R.4; Symbalisty, E.M.D.8; Chanrion, Olivier Arnaud2; Odzimek, A.9; van der Velde, O.7; Neubert, Torsten2
1 Solar System Physics, National Space Institute, Technical University of Denmark2 National Space Institute, Technical University of Denmark3 University of Bath4 SciTech Solutions Ltd5 Los Alamos National Laboratory6 University of Leicester7 Universitat Politècnica de Catalunya8 Los Alamos National Laboratory9 University of Leicester
The electromagnetic radiation emitted by an electron avalanche beam resulting from relativistic runaway breakdown within the Earth's atmosphere is investigated. It is found from theoretical modeling with a computer simulation that the electron beam emits electromagnetic radiation which is characterized by consecutive broadband pulses in the low-frequency radio range from similar to 10 to 300 kHz at a distance of similar to 800 km. Experimental evidence for the existence of consecutive broadband pulses is provided by low-frequency radio observations of sprite-producing lightning discharges at a distance of similar to 550 km. The measured broadband pulses occur similar to 4-9 ms after the sprite-producing lightning discharge, they exhibit electromagnetic radiation which mainly spans the frequency range from similar to 50 to 350 kHz, and they exhibit complex waveforms without the typical ionospheric reflection of the first hop sky wave. Two consecutive pulses occur similar to 4.5 ms and similar to 3 ms after the causative lightning discharge and coincide with the sprite luminosity. It is concluded that relativistic runaway breakdown within the Earth's atmosphere can emit broadband electromagnetic pulses and possibly generates sprites. The source location of the broadband pulses can be determined with an interferometric network of wideband low-frequency radio receivers to lend further experimental support to the relativistic runaway breakdown theory.
Journal of Geophysical Research, 2011, Vol 116, Issue A1