Repozitorij Univerze v Novi Gorici

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Naslov:Radar Sensing of Ultra-High Energy Cosmic Ray Showers
Avtorji:ID Lundquist, Jon Paul, UofU (Avtor), et al.
Datoteke: Gradivo nima datotek, ki so prostodostopne za javnost. Gradivo je morda fizično dosegljivo v knjižnici fakultete, zalogo lahko preverite v COBISS-u. Povezava se odpre v novem oknu
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:2.11 - Diplomsko delo
Organizacija:UNG - Univerza v Novi Gorici
Opis:The intent of this paper is to review the history and potential importance of the use of radar techniques in detecting the ionization columns of ultra-high energy cosmic ray showers and give a short overview of a currently planned radar experiment at the Telescope Array. There is much activity in cosmic ray research to study the composition and source locations of this phenomena. Radar would be an important addition to fluorescence and scintillation detection as it theoretically could attain greater volume coverage and nearly the accuracy of fluorescence systems with less infrastructure and much longer running times. The currently estimated mean echo lifetime is on the order of 50 µs for a cosmic ray of energy 10^19 eV. It is shown that a continuous wave bi-directional radar system transmitting in the low-VHF with a large obstruction between receiver and transmitter (such as a mountain or earth curvature), which assures direct transmission is reduced, is the nominal configuration and the planned radar experiment at the Telescope Array satisfies these requirements.
Ključne besede:cosmic rays, radar
PID:20.500.12556/RUNG-5142-ad994dbf-38dc-321e-6c48-da5ea4044922 Novo okno
COBISS.SI-ID:5615867 Novo okno
NUK URN:URN:SI:UNG:REP:CDOYVGRZ
Datum objave v RUNG:24.04.2020
Število ogledov:2711
Število prenosov:0
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Vaša ocena:Ocenjevanje je dovoljeno samo prijavljenim uporabnikom.
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