First optical observations of energetic electron precipitation at 4278 Å caused by a powerful VLF transmitter. Issue 7 (2nd April 2014)

• Record Type: Journal Article
• Authors: Denton, M. H.; Kosch, M. J.; Borovsky, J. E.; Clilverd, M. A.; Friedel, R. H. W.; Ulich, T.
• Is Part Of: Geophysical research letters. Volume 41:Issue 7(2014:Apr.)
• Page Start: 2237
• Page End: 2242
• Publication Date: 2014-04-02
• Subjects: VLF -- radiation belts; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2014GL059553
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: A summary is presented of experimental optical observations at 4278 Å from close to a powerful (~150 kW) VLF transmitter (call sign JXN) with a transmission frequency of 16.4 kHz. Approximately 2.5 s after transmitter turn‐on, a sudden increase in optical emissions at 4278 Å was detected using a dedicated camera/charge‐coupled device (CCD) monitoring system recording at a frequency of 10 Hz. The optical signal is interpreted as a burst of electron precipitation lasting ~0.5 s, due to gyro‐resonant wave‐particle interactions between the transmitted wave and the magnetospheric electron population. The precipitation was centered on the zenith and had no detectable spatial structure. The timing of this sequence of events is in line with theoretical predictions and previous indirect observations of precipitation. This first direct measurement of VLF‐induced precipitation at 4278 Å reveals the spatial and temporal extent of the resulting optical signal close to the transmitter. Key Points: Energetic electrons detected at turn‐on of high‐power VLF transmitter All-sky burst of electrons lasts at least 0.5 s First direct optical confirmation of electron precipitation at 4278 Å