A 3-year sample of almost 1,600 elves recorded above South America by the Pierre Auger Cosmic-Ray observatory

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F20%3A00534383" target="_blank" >RIV/68378271:_____/20:00534383 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/00216208:11320/20:10421852 RIV/61989592:15310/20:73601433

Výsledek na webu

<a href="http://hdl.handle.net/11104/0312588" target="_blank" >http://hdl.handle.net/11104/0312588</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1029/2019EA000582" target="_blank" >10.1029/2019EA000582</a>

Jazyk výsledku

angličtina

Název v původním jazyce

A 3-year sample of almost 1,600 elves recorded above South America by the Pierre Auger Cosmic-Ray observatory

Popis výsledku v původním jazyce

Elves are a class of transient luminous events, with a radial extent typically greater than 250km, that occur in the lower ionosphere above strong electrical storms. We report the observation of 1,598 elves, from 2014 to 2016, recorded with unprecedented time resolution (100 ns) using the fluorescence detector (FD) of the Pierre Auger Cosmic-Ray Observatory. The Auger Observatory is located in the Mendoza province of Argentina with a viewing footprint for elve observations of 3106km 2, reaching areas above the Pacific and Atlantic Oceans, as well as the Cordoba region, which is known for severe convective thunderstorms. Primarily designed for ultrahigh energy cosmic-ray observations, the Auger FD turns out to be very sensitive to the ultraviolet emission in elves.

Název v anglickém jazyce

A 3-year sample of almost 1,600 elves recorded above South America by the Pierre Auger Cosmic-Ray observatory

Popis výsledku anglicky

Elves are a class of transient luminous events, with a radial extent typically greater than 250km, that occur in the lower ionosphere above strong electrical storms. We report the observation of 1,598 elves, from 2014 to 2016, recorded with unprecedented time resolution (100 ns) using the fluorescence detector (FD) of the Pierre Auger Cosmic-Ray Observatory. The Auger Observatory is located in the Mendoza province of Argentina with a viewing footprint for elve observations of 3106km 2, reaching areas above the Pacific and Atlantic Oceans, as well as the Cordoba region, which is known for severe convective thunderstorms. Primarily designed for ultrahigh energy cosmic-ray observations, the Auger FD turns out to be very sensitive to the ultraviolet emission in elves.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2020

Kód důvěrnosti údajů

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

Název periodika

Earth and Space Science

ISSN

2333-5084

e-ISSN

—

Svazek periodika

7

Číslo periodika v rámci svazku

4

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

17

Strana od-do

1-17

Kód UT WoS článku

000534600100003

EID výsledku v databázi Scopus

2-s2.0-85083673851