EGU23-9381
https://doi.org/10.5194/egusphere-egu23-9381
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

The scientific payload of the ALOFT mission to chase Terrestrial Gamma-ray Flashes and gamma-ray glows

Martino Marisaldi1, Nikolai Østgaard1, Kjetil Ullaland1, Shiming Yang1, B. Hasan Qureshi1, Jens Søndergaard1, Andrey Mezentsev1, David Sarria1, Nikolai Lehtinen1, Timothy J. Lang2, Hugh Christian3, Mason Quick2, Richard Blakeslee2, J. Eric Grove4, and Daniel Shy5
Martino Marisaldi et al.
  • 1University of Bergen, Birkeland Centre for Space Science, Department of Physics and Technology, Bergen, Norway (martino.marisaldi@uib.no)
  • 2NASA Marshall Space Flight Center, Huntsville, USA
  • 3Department of Atmospheric Science, Earth System Science Center, University of Alabama in Huntsville, Huntsville, USA
  • 4U.S. Naval Research Laboratory, Washington DC, USA
  • 5National Research Council Research Associate resident at the U.S. Naval Research Laboratory, Washington DC, 20375, USA

ALOFT (Airborne Lightning Observatory for FEGS and TGFs) is a flight campaign designed to observe Terrestrial Gamma-ray Flashes (TGF) and gamma-ray glows close to their production source. The campaign consists of 50 flight hours of a NASA ER-2 research aircraft taking off from Florida and is scheduled for July 2023. The ER-2 cruise altitude of 20 km allows flying over active thunderstorms in the Gulf of Mexico and Caribbean region, one of the most TGF-active region on the planet. The main challenge for TGF detection at close distance is the large variability in the expected gamma-ray flux, spanning four orders of magnitude depending on the radial distance from the source. To cope with this challenge, the ALOFT gamma-ray payload consists of several detectors of different size, made of different materials and readout sensors, designed to cover 4 orders of magnitude dynamic range on the typical TGF/gamma-ray glow energy range (~100 keV - ~40 MeV). In addition, the payload includes the Fly’s Eye GLM Simulator (FEGS), an array of imaging photometers sensitive at different wavelengths, and electric field change meters, and the Lightning Instrument Package (LIP), giving three component electric field measurements. The synergy between airborne gamma-ray, optical and electric field measurements, combined with ground-based radio observations, will provide a unique set of observations to constrain the source properties and their physics. This presentation will focus on the ALOFT scientific payload and the system architecture.

How to cite: Marisaldi, M., Østgaard, N., Ullaland, K., Yang, S., Qureshi, B. H., Søndergaard, J., Mezentsev, A., Sarria, D., Lehtinen, N., Lang, T. J., Christian, H., Quick, M., Blakeslee, R., Grove, J. E., and Shy, D.: The scientific payload of the ALOFT mission to chase Terrestrial Gamma-ray Flashes and gamma-ray glows, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-9381, https://doi.org/10.5194/egusphere-egu23-9381, 2023.