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Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs
Published on: August 27, 2019
The Temporal Relationship Between Terrestrial Gamma-Ray Flashes and Associated Optical Pulses From Lightning
C A Skeie1, N Østgaard1, A Mezentsev1
1Birkeland Centre for Space Science Institute of Physics and Technology University of Bergen Bergen Norway.
Researchers analyzed 221 Terrestrial Gamma-ray Flashes (TGFs) and optical pulses using the ASIM instrument. They found TGF onsets precede optical pulses, with longer TGFs showing greater delays, suggesting distinct emission mechanisms.
Area of Science:
- Atmospheric physics
- Space science
- High-energy astrophysics
Background:
- Terrestrial Gamma-ray Flashes (TGFs) are brief, intense bursts of gamma rays originating from thunderstorms.
- Understanding the relationship between TGFs and optical emissions is crucial for comprehending lightning processes.
Purpose of the Study:
- To investigate the temporal relationship between TGFs and associated optical pulses observed by the ASIM instrument.
- To categorize TGF events based on their duration and the delay between TGF and optical pulse onsets.
Main Methods:
- Analysis of 221 TGF events detected by the Atmosphere-Space Interactions Monitor (ASIM) on the International Space Station.
- Utilizing X- and gamma-ray energy detections, photometer data (180-230, 337, 777 nm), and optical camera data (337, 777 nm).
- Cross-referencing TGF characteristics and lightning detections to determine event association and location relative to the ASIM photometer's field of view.
Main Results:
- 72 out of 221 events showed clear association between TGFs and optical pulses within the photometer's field of view.
- TGF onsets consistently occurred before or simultaneously with optical pulse onsets, accounting for cloud scattering effects.
- A correlation was observed between longer TGF durations and increased delays in optical pulse onsets.
- Two distinct event groups emerged: one with potential overlap between TGF and optical emissions, and another with significant delays unexplainable by cloud scattering.
Conclusions:
- TGFs and associated optical emissions exhibit complex temporal relationships.
- The observed delays and durations suggest at least two different mechanisms may be responsible for generating TGFs and their optical counterparts.
- Further research is needed to fully elucidate the interplay between high-energy atmospheric phenomena and visible light emissions during thunderstorms.
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