Increase of onboard aircraft exposure level during a solar flare.
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F03%3A49035184" target="_blank" >RIV/61389005:_____/03:49035184 - isvavai.cz</a>
Výsledek na webu
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DOI - Digital Object Identifier
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Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Increase of onboard aircraft exposure level during a solar flare.
Popis výsledku v původním jazyce
Si-diode spectrometer has been used for long-term monitoring of the exposure level onboard of an CSA a.s. aircraft between 22nd March and 7th May 2001. The 15th April at 13 h 50 of universal time a rather intense solar flare has been registered by on-Earth cosmic radiation monitor station, The Ground level event numbered 60. At this time, the aircraft with equipment mentioned onboard was flying from Prague to New York. After the end of monitoring period, an increase of onboard exposure level has been really identified in the record of measurements. The directly registered date showed an increase of about factor of two as compared to only galactic cosmic radiation, both in the rate number of impulses as well as in dose-rate absorbed in Si. The date showed also that the event spectra during the flare are different as compared to galactic radiation .
Název v anglickém jazyce
Increase of onboard aircraft exposure level during a solar flare.
Popis výsledku anglicky
Si-diode spectrometer has been used for long-term monitoring of the exposure level onboard of an CSA a.s. aircraft between 22nd March and 7th May 2001. The 15th April at 13 h 50 of universal time a rather intense solar flare has been registered by on-Earth cosmic radiation monitor station, The Ground level event numbered 60. At this time, the aircraft with equipment mentioned onboard was flying from Prague to New York. After the end of monitoring period, an increase of onboard exposure level has been really identified in the record of measurements. The directly registered date showed an increase of about factor of two as compared to only galactic cosmic radiation, both in the rate number of impulses as well as in dose-rate absorbed in Si. The date showed also that the event spectra during the flare are different as compared to galactic radiation .
Klasifikace
Druh
J<sub>x</sub> - 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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Návaznosti výsledku
Projekt
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Návaznosti
Z - Vyzkumny zamer (s odkazem do CEZ)
Ostatní
Rok uplatnění
2003
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Bezpečnost jaderné energie
ISSN
1210-7085
e-ISSN
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Svazek periodika
11
Číslo periodika v rámci svazku
3/4
Stát vydavatele periodika
CZ - Česká republika
Počet stran výsledku
5
Strana od-do
103-107
Kód UT WoS článku
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EID výsledku v databázi Scopus
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