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Naslov:Raman LIDARs and atmospheric calibration along the line-of-sight of the Cherenkov Telescope Array
Avtorji:ID Stanič, Samo, University of Nova Gorica (Avtor)
ID Wang, Longlong, University of Nova Gorica (Avtor)
ID Zavrtanik, Marko, Jožef Stefan Institute (Avtor), et al.
Datoteke:.pdf ICRC2019_814.pdf (1,29 MB)
MD5: 66652250F237A05D98667458C145448A
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. Employing more than 100 (north and south sites) Imaging Atmospheric Cherenkov Telescopes in the northern and southern hemispheres, it was designed to reach unprecedented sensitivity and energy resolution. Understanding and correcting for systematic biases on the absolute energy scale and instrument response functions will be a cru- cial issue for the performance of CTA. The Montpellier group and the Spanish/Italian/Slovenian collaboration are currently building two Raman LIDAR prototypes for the online atmospheric cal- ibration along the line-of-sight of the CTA. Requirements for such a solution include the ability to characterize aerosol extinction at two wavelengths to distances up to 30 km with an accuracy better than 5%, within exposure time scales of about a minute, steering capabilities and close interaction with the CTA array control and data acquisition system as well as other auxiliary in- struments. Our Raman LIDARs have design features that make them different from those used in atmospheric science and are characterized by large collecting mirrors (∼2.5 m 2 ), liquid light- guides that collect the light at the focal plane and transport it to the readout system, reduced acquisition time and highly precise Raman spectrometers. The Raman LIDARs will participate in a cross-calibration and characterization campaign of the atmosphere at the CTA North site at La Palma, together with other site characterization instruments. After a one-year test period there, an in-depth evaluation of the solutions adopted by the two projects will lead to a final Raman LIDAR design proposal for both CTA sites.
Ključne besede:Raman lidar atmospheric calibration Cherenkov Telescope Array
Verzija publikacije:Objavljena publikacija
Leto izida:2019
Št. strani:8
Številčenje:814
PID:20.500.12556/RUNG-4709-5a3e2158-1787-a90a-764f-10fc5bee3a5b Novo okno
COBISS.SI-ID:5444347 Novo okno
NUK URN:URN:SI:UNG:REP:RIGTKVKS
Datum objave v RUNG:29.08.2019
Število ogledov:4983
Število prenosov:104
Metapodatki:XML DC-XML DC-RDF
:
STANIČ, Samo, WANG, Longlong in ZAVRTANIK, Marko, 2019, Raman LIDARs and atmospheric calibration along the line-of-sight of the Cherenkov Telescope Array. V : 36th International Cosmic Ray Conference -ICRC2019 [na spletu]. Objavljeni znanstveni prispevek na konferenci. 2019. [Dostopano 12 april 2025]. Pridobljeno s: https://repozitorij.ung.si/IzpisGradiva.php?lang=slv&id=4709
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Gradivo je del zbornika

Naslov:36th International Cosmic Ray Conference -ICRC2019

Gradivo je del revije

Naslov:proceedings of science
Leto izida:2019

Licence

Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
Opis:Najbolj omejujoča licenca Creative Commons. Uporabniki lahko prenesejo in delijo delo v nekomercialne namene in ga ne smejo uporabiti za nobene druge namene.
Začetek licenciranja:29.08.2019

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