Non-uniform ionisation of the upper atmosphere due to the electromagnetic pulse from a horizontal lightning discharge

Details Non-uniform ionisation of the upper atmosphere due to the electromagnetic pulse from a horizontal lightning discharge Non-uniform ionisation of the upper atmosphere due to the electromagnetic pulse from a horizontal lightning discharge

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jastp..63..559c&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 63, Issue 6, p. 559-580.

Physics

21

Scientific paper

The purpose of this paper is to model numerically the ionisation created in the mesosphere above a strong horizontal (cloud-to-cloud) lightning discharge, and thus to understand better the formation of elves and related columniform (spatially structured) sprites. Such ionisation depends upon height, via the ratio of the VLF//LF wave electric field (radiated by the current in the discharge) to the atmospheric neutral density. The simulation shows local maxima on the order of 10 km apart due to the interference between direct waves radiated by the discharge current, waves reflected by the ground and waves reflected by the ionosphere. Parametric studies are carried out varying the frequency, amplitude, height, length and duration of the current. For waves >=30kHz generated by a current >=50kA, localised peaks of electron density occur from 75 to 85km altitude, particularly for discharges longer than 15 km. From such peaks, time-varying ``stalactites'' on the bottom of the ionosphere, streamers could develop and propagate downwards. These could become columniform sprites in the presence of the quasi-electrostatic field due to the negative charge remaining in the thundercloud after a positive cloud-to-ground discharge.

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