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

Kód výsledku v 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>

Výsledek na webu

<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>

Jazyk výsledku

angličtina

Název v původním jazyce

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

Popis výsledku v původním jazyce

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.

Název v anglickém jazyce

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

Popis výsledku anglicky

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.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2019

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

EPJ Web of Conferences

ISBN

—

ISSN

2100-014X

e-ISSN

2100-014X

Počet stran výsledku

3

Strana od-do

1-3

Název nakladatele

EDP Sciences

Místo vydání

Les Ulis

Místo konání akce

Catania

Datum konání akce

12. 6. 2018

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000570244200033