EGU25-4072, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-4072
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Wednesday, 30 Apr, 16:35–16:45 (CEST)
 
Room 1.31/32
Upcoming broadband electromagnetic balloon measurements related to terrestrial gamma ray flashes and gamma glows 
Ivana Kolmasova1,2, Ondrej Santolik1,2, Sébastien Celestin3, Eric Defer4, and Radek Lan1
Ivana Kolmasova et al.
  • 1Institute of Atmospheric Physics CAS, department of Space Physics, Prague, Czechia (iko@ufa.cas.cz)
  • 2Faculty of Mathematics and Physics, Charles University, Prague, Czechia
  • 3LPC2E, University of Orleans, CNRS, Orléans, France
  • 4Laboratoire d’Aérologie, Université de Toulouse, CNRS, OMP, UPS, Toulouse, France

Thunderclouds and lightning produce high-energy radiation over a wide range of time scales. Terrestrial gamma-ray flashes (TGFs) are brief emissions lasting ~100 µs, consisting of photons with energies ranging from 20 keV to 40 MeV. Simultaneous ground-based measurements of electromagnetic fields and gamma-ray emissions have found TGFs to be associated with the evolutionary phases of both intracloud and cloud-to-ground lightning discharges.

Gamma-ray glows, on the other hand, last from a few seconds to several tens of minutes, typically coincide with the passage of thunderclouds, and are sometimes abruptly terminated by nearby lightning. Photons emitted during gamma-ray glows share the same energy spectrum as TGFs but are less intense. It was recently discovered that thundercloud regions can glow for hours and that gamma glows are more dynamic phenomena than originally thought.

Both types of gamma-ray emissions are believed to be generated via bremsstrahlung by energetic runaway electrons accelerated in the strong electric fields within thunderclouds. However, the connection between TGFs and gamma-ray glows remains not fully understood.

Until now, the only simultaneous gamma ray and radio wave measurements were conducted onboard an airplane during the ALOFT campaign. The TARANIS mission, which was intended to carry a unique set of electromagnetic, particle, gamma ray, and optical instruments, was unfortunately lost due to the failure of the Vega launcher in 2020.

The STRATELEC balloon project (part of the French-US STRATEOLE-2 project of long-duration balloon flights at the tropical tropopause), with precise synchronization of broadband electric field measurements and a gamma-ray detector, will provide a unique opportunity to correlate individual photon detections with electromagnetic pulses emitted by various lightning processes. These coordinated measurements could help answer the following questions:

  • a) At which stage of the evolution of lightning discharges are TGFs produced?
  • b) Which types of intracloud discharges produce detectable high-energy radiation?
  • c) What are the differences in the electromagnetic signatures of lightning processes associated with TGFs and gamma glows?
  • d) What are the temporal variations in electromagnetic emissions associated with gamma glows?
  • e) Are flickering TGFs truly radio silent?

In this presentation, we introduce the FPGA-based radio receiver RIP (Radio Instrument Package), developed for the STRATELEC balloon project. The receiver is designed to capture and analyze the electromagnetic signatures of various lightning phenomena associated with gamma-ray production, including leader pulses, initial breakdown pulses, compact intracloud discharges, and dart-stepped leader pulses. The anticipated launch is late 2026.

How to cite: Kolmasova, I., Santolik, O., Celestin, S., Defer, E., and Lan, R.: Upcoming broadband electromagnetic balloon measurements related to terrestrial gamma ray flashes and gamma glows , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4072, https://doi.org/10.5194/egusphere-egu25-4072, 2025.