Spectral Observations of Optical Emissions Associated With Terrestrial Gamma‐Ray Flashes
Matthias Heumesser, Olivier Chanrion, Torsten Neubert, Hugh J. Christian, Krystallia Dimitriadou, Francisco J. Gordillo‐Vázquez, Alejandro Luque, Francisco J. Pérez‐Invernón, Richard J. Blakeslee, Nikolai Østgaard, V. Reglero, Christoph Köhn
Abstract
The Atmosphere-Space Interactions Monitor measures Terrestrial Gamma-Ray Flashes (TGFs) simultaneously with optical emissions from associated lightning activity. We analyzed optical measurements at 180-230, 337, and 777.4 nm related to 69 TGFs observed between June 2018 and October 2019. All TGFs are associated with optical emissions and 90% of them are at the onset of a large optical pulse, suggesting that they are connected with the initiation of current surges. A model of photon delay induced by cloud scattering suggests that the sources of the optical pulses are from 0.7 ms before to 4.4 ms after the TGFs, with a median of -10 ± 80 µs, and 1-5 km below the cloud top. The pulses have rise times comparable to lightning but longer durations. Pulse amplitudes at 337 nm are ∼3 times larger than at 777.4 nm. The results support the leader-streamer mechanism for TGF generation.