Measurements of Ionizing Radiation Generated in Thunderstorms
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F23%3A00572948" target="_blank" >RIV/61389005:_____/23:00572948 - isvavai.cz</a>
Alternative codes found
RIV/68407700:21230/23:00371105 RIV/68407700:21340/23:00371105
Result on the web
<a href="http://dx.doi.org/10.1109/AERO55745.2023.10115668" target="_blank" >http://dx.doi.org/10.1109/AERO55745.2023.10115668</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1109/AERO55745.2023.10115668" target="_blank" >10.1109/AERO55745.2023.10115668</a>
Alternative languages
Result language
angličtina
Original language name
Measurements of Ionizing Radiation Generated in Thunderstorms
Original language description
Measurements and theoretical studies show that thunderclouds can act as particle accelerators in nature. Terrestrial gamma ray flashes (TGFs) are bursts of gamma rays with energies ranging from below 10 keV to above 40 MeV, which last for microseconds to several milliseconds, and coincide with lightning produced in Earth's atmosphere. The gamma-ray spectra of TGFs are consistent with bremsstrahlung from energetic electrons going upward into space. More recently, similar phenomena but beamed downward have been discovered by ground-based observations: short bursts, 'downward TGFs', with durations of milliseconds and long bursts, 'thunderstorm ground enhancements' (TGEs) or gamma ray glows, with durations up to several minutes. These findings have established a new academic field called 'high-energy atmospheric physics'. The origin, and exact mechanisms creating the thunderstorm radiation (TGFs and TGEs), are still unclear but it has been suggested that TGFs are caused by intense electric fields produced above or inside thunderstorms. To explain TGF, electrons which are traveling at speeds very close to the speed of light collide with atomic nuclei in the atmosphere and release their energy in the form of X-rays (bremsstrahlung). Large populations of energetic electrons can be formed by avalanche growth driven by electric fields, a phenomenon called relativistic runaway electron avalanche (RREA). Airplane crew and passengers flying near thunderstorms could therefore be exposed to 'dangerously' high levels of radiation in the form of short terrestrial y-ray flashes and little longer y-ray glows. To clarify the origin of TGFs, and to evaluate the absorbed dose of thunderstorm radiation, the project CRREAT (Research Centre of Cosmic Rays and Radiation Events in Atmosphere) measures both the lightning and the ionizing radiation during thunderstorms using detection instrument mounted on the roofs and inside of cars, and with ionizing radiation detectors installed on high mountains. One other important research area of CRREAT is measurements and simulations of the radiation field at aviation altitudes and at low earth orbits (LEO), since this poses a health risk for crew members and passenger's onboard aircraft and spacecraft. This paper gives an overview of possible sources of ionizing radiation and phenomena during thunderstorm.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10509 - Meteorology and atmospheric sciences
Result continuities
Project
<a href="/en/project/EF15_003%2F0000481" target="_blank" >EF15_003/0000481: Research Center of Cosmic Rays and Radiation Events in the Atmosphere</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
IEEE Aerospace Conference Proceedings
ISBN
978-1-6654-9032-0
ISSN
1095-323X
e-ISSN
—
Number of pages
10
Pages from-to
5668
Publisher name
IEEE
Place of publication
Big Sky
Event location
Big Sky
Event date
Mar 4, 2023
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
001008282002002