dc.creator | Ballester, Otger | es |
dc.creator | Blanch, Oscar | es |
dc.creator | Boix, Joan | es |
dc.creator | Bregeon, Johan | es |
dc.creator | Brun, Patrick | es |
dc.creator | Çolak, §ıdıka Merve | es |
dc.creator | Doro, Michele | es |
dc.creator | Da Deppo, Vania | es |
dc.creator | Font, Lluís | es |
dc.creator | Gabella, Omar | es |
dc.creator | García-Tenorio García-Balmaseda, Rafael | es |
dc.creator | Gaug, Markus | es |
dc.creator | Maggio, Camilla | es |
dc.creator | Martínez, Manel Cruz | es |
dc.creator | Martínez, Óscar | es |
dc.creator | Adrover, Pere Munar | es |
dc.creator | Ramos, Raúl | es |
dc.creator | Rivoire, Stephane | es |
dc.creator | Staniˇc, Samo | es |
dc.creator | Villar, David | es |
dc.creator | Vasileiadis, George | es |
dc.creator | Wang, Longlong | es |
dc.creator | Zavrtanik, Marko | es |
dc.date.accessioned | 2020-07-23T11:45:59Z | |
dc.date.available | 2020-07-23T11:45:59Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | Ballester, O., Blanch, O., Boix, J., Bregeon, J., Brun, P., Çolak, §.M.,...,Zavrtanik, M. (2019). Raman LIDARs for the atmospheric calibrationalong the line-of-sight of CTA. En 36th International Cosmic Ray Conference, Madison, Wisconsin, EE. UU.. | |
dc.identifier.uri | https://hdl.handle.net/11441/99780 | |
dc.description.abstract | The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory forgamma-ray astronomy at very-high energies. Employing more than 100 Imaging AtmosphericCherenkov Telescopes in the northern and southern hemispheres, it was designed to reach un-precedented sensitivity and energy resolution. Understanding and correcting for systematic bi-ases on the absolute energy scale and instrument response functions will be a crucial issue forthe performance of CTA. The LUPM group and the Spanish/Italian/Slovenian collaboration arecurrently building two Raman LIDAR prototypes for the online atmospheric calibration alongthe line-of-sight of the CTA. Requirements for such a solution include the ability to characterizeaerosol extinction at two wavelengths to distances of 30 km with an accuracy better than 5%,within time scales of about a minute, steering capabilities and close interaction with the CTAarray control and data acquisition system as well as other auxiliary instruments. Our Raman LI-DARs have design features that make them different from those used in atmospheric science andare characterized by large collecting mirrors (∼2.5 m2), liquid light-guides that collect the light atthe focal plane and transport it to the readout system, reduced acquisition time and highly preciseRaman spectrometers. The Raman LIDARs will participate in a cross-calibration and character-ization campaign of the atmosphere at the CTA North site at La Palma, together with other sitecharacterization instruments. After a one-year test period there, an in-depth evaluation of the so-lutions adopted by the two projects will lead to a final Raman LIDAR design proposal for bothCTA sites. | es |
dc.format | application/pdf | es |
dc.format.extent | 9 p. | es |
dc.language.iso | eng | es |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | Raman LIDARs for the atmospheric calibrationalong the line-of-sight of CTA | es |
dc.type | info:eu-repo/semantics/conferenceObject | es |
dcterms.identifier | https://ror.org/03yxnpp24 | |
dc.type.version | info:eu-repo/semantics/publishedVersion | es |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | es |
dc.contributor.affiliation | Universidad de Sevilla. Departamento de Física Aplicada II | es |
dc.relation.publisherversion | https://pos.sissa.it/358/814/pdf | es |
dc.publication.initialPage | 1 | es |
dc.publication.endPage | 7 | es |
dc.eventtitle | 36th International Cosmic Ray Conference | es |
dc.eventinstitution | Madison, Wisconsin, EE. UU. | es |