A rotationally symmetric lateral distribution function for radio emission from inclined air showers

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00549256" target="_blank" >RIV/68378271:_____/19:00549256 - isvavai.cz</a>
Result on the web
<a href="https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_03009.pdf" target="_blank" >https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_03009.pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/epjconf/201921603009" target="_blank" >10.1051/epjconf/201921603009</a>

Result language
angličtina
Original language name
A rotationally symmetric lateral distribution function for radio emission from inclined air showers
Original language description
Radio detection of inclined air showers is currently receiving great attention. To exploit the potential, a suitable event reconstruction needs to be developed. A crucial step in this direction is the development of a model for the lateral distribution of the radio signals, which in the case of inclined air showers exhibits asymmetries due to “early late” effects in addition to the usual asymmetries from the superposition of charge-excess and geomagnetic emission. We present a model which corrects for all asymmetries and successfully describes the lateral distribution of the energy fluence with a rotationally symmetric function. This gives access to the radiation energy as a measure of the energy of the cosmic -ray primary, and is also sensitive to the depth of the shower maximum.
Czech name
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Czech description
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Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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