Detections of high peak current lightning and observations of Elves
- 1Birkeland Centre for Space Science, University of Bergen, Norway
- 2Instituto de Astrofisica de Andalucia, CSIC, Granada, Spain
- 3National Space Institute, Technical University of Denmark, Denmark
- 4University of Valencia, Spain
Elves are produced when electromagnetic pulses from lightning interact with the lower parts of the ionosphere and are observed from space as expanding rings of light in the UV and visible optical bands. Elves are known to be associated with high peak current lightning. Using data from the Modular Multi-spectral Imaging Array (MMIA) instrument of the Atmosphere-Space Interactions Monitor (ASIM) payload, we search for observations of Elves when high peak currents (>70 kA) are detected by the global ground-based lightning detection network GLD360. We identify two types of events; high peak current detections associated with Elves, and high peak current detections not associated with Elves. To understand why some high peak current discharges do not generate observable Elves, we explore the number of lightning discharges and their peak currents leading up to the events. Preliminary results indicate that for current pulses with peak currents below 100 kA we observe a significant number of Elves, but this quantity depends on the lightning activity within 5 minutes before. Current pulses with peak currents above 120 kA nearly always produce Elves, regardless of the preceding lightning activity.
How to cite: Bjørge-Engeland, I., Østgaard, N., Marisaldi, M., Luque, A., Mezentsev, A., Lehtinen, N., Chanrion, O., Neubert, T., and Reglero, V.: Detections of high peak current lightning and observations of Elves, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-9415, https://doi.org/10.5194/egusphere-egu23-9415, 2023.