Radio Frequency Electromagnetic Radiation From Streamer Collisions. Issue 19 (12th October 2017)

• Record Type: Journal Article
• Authors: Luque, Alejandro
• Is Part Of: Journal of geophysical research. Volume 122:Issue 19(2017)
• Page Start: 10, 497
• Page End: 10, 509
• Publication Date: 2017-10-12
• Subjects: streamers -- high‐energy atmospheric physics -- radio frequency -- FDTD; Atmospheric physics -- Periodicals; Geophysics -- Periodicals; 551.5
• DOI: 10.1002/2017JD027157
• Languages: English
• ISSNs: 2169-897X

Abstract

Abstract: We present a full electromagnetic model of streamer propagation where the Maxwell equations are solved self‐consistently together with electron transport and reactions including photoionization. We apply this model to the collision of counter‐propagating streamers in gaps tens of centimeters wide and with large potential differences of hundreds of kilovolts. Our results show that streamer collisions emit electromagnetic pulses that, at atmospheric pressure, dominate the radio frequency spectrum of an extended corona in the range from about 100 MHz to a few gigahertz. We also investigate the fast penetration, after a collision, of electromagnetic fields into the streamer heads and show that these fields are capable of accelerating electrons up to about 100 keV. By substantiating the link between X‐rays and high‐frequency radio emissions and by describing a mechanism for the early acceleration of runaway electrons, our results support the hypothesis that streamer collisions are essential precursors of high‐energy processes in electric discharges. Plain Language Summary: Long electric discharges such as a lightning stroke simultaneously produce bursts of X‐rays and radio frequency noise. Here we present a numerical model that explains this coincidence by attributing both phenomena to the collisions of counter‐propagating conducting filaments called "streamers." Key Points: We present a streamer model with electromagnetic propagation, electron transport, impact ionization, attachment, and photoionization The radiated field of a corona is likely dominated in the UHF range by the electromagnetic pulses emitted by streamer collisions The electric field that, after a streamer collision, penetrates into each streamer is capable of accelerating electrons up to 100 keV