Premium
Relativistic electron beam propagation in the Earth's atmosphere: Modeling results
Author(s) -
Neubert T.,
Gilchrist B.,
Wilderman S.,
Habash L.,
Wang H. J.
Publication year - 1996
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/96gl00247
Subject(s) - thermosphere , physics , computational physics , atmosphere (unit) , monte carlo method , electron , atmosphere of earth , beam (structure) , ionosphere , geophysics , atmospheric sciences , meteorology , nuclear physics , optics , statistics , mathematics
Linear accelerators (linacs), capable of producing 5 M e V energy electron beams at 80 m A currents, are now down to a size that allow them to be flown on sounding rockets or balloons. This opens up new opportunities for atmospheric/ionospheric modification experiments where the mesosphere and thermosphere regions of the atmosphere can be perturbed down to 40 km altitude. In this paper beam propagation and atmospheric perturbation effects are studied by Monte Carlo simulations and by analytical means. It is shown that the earth' magnetic field severely limits the radial expansion of the beam otherwise induced by electron‐neutral collisions. It is also shown that the so‐called “envelope‐equations” from high‐energy laboratory physics adequately describe beam propagation in the upper atmosphere. The plasma density and electric conductivity modifications to the atmosphere are calculated from the Monte Carlo simulations. Inside the beam the conductivity in the 40–50 km altitude region is enhanced more than one order of magnitude by a 10 µs‐duration pulse. Some ideas for future scientific investigations are discussed, including the generation of electrical discharges by beams injected over thunderstorm regions.