Characterization of the radiation environment by liulin-type spectrometers

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F11%3A00360649" target="_blank" >RIV/61389005:_____/11:00360649 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1093/rpd/ncq534" target="_blank" >http://dx.doi.org/10.1093/rpd/ncq534</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1093/rpd/ncq534" target="_blank" >10.1093/rpd/ncq534</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Characterization of the radiation environment by liulin-type spectrometers

Popis výsledku v původním jazyce

Liulin-type spectrometers can characterise the type of predominant particles and their energy in the radiation environment. The results from calibrations and space and aircraft experiments revealed that the most informative is by the shape of the deposited energy spectrum. Spectra generated by galactic cosmic rays (GCR) protons and their secondaries look like straight lines in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions, these spectra are similar to the GCR spectra. All types ofspectra have a knee close to 6.3 MeV of deposited energy, which corresponds to the stopping energy of protons in the detector.

Název v anglickém jazyce

Characterization of the radiation environment by liulin-type spectrometers

Popis výsledku anglicky

Liulin-type spectrometers can characterise the type of predominant particles and their energy in the radiation environment. The results from calibrations and space and aircraft experiments revealed that the most informative is by the shape of the deposited energy spectrum. Spectra generated by galactic cosmic rays (GCR) protons and their secondaries look like straight lines in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions, these spectra are similar to the GCR spectra. All types ofspectra have a knee close to 6.3 MeV of deposited energy, which corresponds to the stopping energy of protons in the detector.

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BG - Jaderná, atomová a molekulová fyzika, urychlovače

OECD FORD obor

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Projekt

—

Návaznosti

Z - Vyzkumny zamer (s odkazem do CEZ)

Rok uplatnění

2011

Kód důvěrnosti údajů

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

Název periodika

Radiation Protection Dosimetry

ISSN

0144-8420

e-ISSN

—

Svazek periodika

144

Číslo periodika v rámci svazku

1

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

4

Strana od-do

680-683

Kód UT WoS článku

000289164200147

EID výsledku v databázi Scopus

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