Preliminary results from the Latin American Giant Observatory space weather simulation chain

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549297" target="_blank" >RIV/68378271:_____/18:00549297 - isvavai.cz</a>

Výsledek na webu

<a href="https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1002/2017SW001774" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1002/2017SW001774</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1002/2017SW001774" target="_blank" >10.1002/2017SW001774</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Preliminary results from the Latin American Giant Observatory space weather simulation chain

Popis výsledku v původním jazyce

The Space Weather program of the Latin American Giant Observatory (LAGO) Collaboration was designed to study the variation of the flux of atmospheric secondary particles at ground level produced during the interaction of cosmic rays with the air. This work complements and expands the inference capabilities of the LAGO detection network to identify the influence of solar activity on the particle flux, at places having different geomagnetic rigidity cut-offs and atmospheric depths. This program is developed through a series of Monte Carlo sequential simulations to compute the intensity spectrum of the various components of the radiation field on the ground. A key feature of these calculations is that we performed detailed radiation transport computations as a function of incident direction, time, altitude, and latitude and longitude.n

Název v anglickém jazyce

Preliminary results from the Latin American Giant Observatory space weather simulation chain

Popis výsledku anglicky

The Space Weather program of the Latin American Giant Observatory (LAGO) Collaboration was designed to study the variation of the flux of atmospheric secondary particles at ground level produced during the interaction of cosmic rays with the air. This work complements and expands the inference capabilities of the LAGO detection network to identify the influence of solar activity on the particle flux, at places having different geomagnetic rigidity cut-offs and atmospheric depths. This program is developed through a series of Monte Carlo sequential simulations to compute the intensity spectrum of the various components of the radiation field on the ground. A key feature of these calculations is that we performed detailed radiation transport computations as a function of incident direction, time, altitude, and latitude and longitude.n

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2018

Kód důvěrnosti údajů

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

Název periodika

Space Weather-the International Journal of Research and Applications

ISSN

1542-7390

e-ISSN

1542-7390

Svazek periodika

16

Číslo periodika v rámci svazku

5

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

15

Strana od-do

461-475

Kód UT WoS článku

000435285400004

EID výsledku v databázi Scopus

2-s2.0-85046772737