Atmospheric monitoring for very high energy gamma energy cherenkov telescopes based on HSRL: Development of high accuracy non-invasive etalon characterization techniques

Maltezos, S; Fokitis, E; Gika, V; Maragos, N; Koubli, E; Koutsourakis, G; Aravantinos, A

dc.contributor.author	Maltezos, S	en
dc.contributor.author	Fokitis, E	en
dc.contributor.author	Gika, V	en
dc.contributor.author	Maragos, N	en
dc.contributor.author	Koubli, E	en
dc.contributor.author	Koutsourakis, G	en
dc.contributor.author	Aravantinos, A	en
dc.date.accessioned	2014-03-01T01:35:21Z
dc.date.available	2014-03-01T01:35:21Z
dc.date.issued	2011	en
dc.identifier.issn	09205632	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/21009
dc.subject	Very High Energy	en
dc.title	Atmospheric monitoring for very high energy gamma energy cherenkov telescopes based on HSRL: Development of high accuracy non-invasive etalon characterization techniques	en
heal.type	journalArticle	en
heal.identifier.primary	10.1016/j.nuclphysbps.2011.04.026	en
heal.identifier.secondary	http://dx.doi.org/10.1016/j.nuclphysbps.2011.04.026	en
heal.publicationDate	2011	en
heal.abstract	In the framework of the design of a High Spectral Resolution Lidar (HSRL), a prototype receiver telescope based on a massive parabolic mirror is presented in this work. We also describe performance tests of three available etalons in resolving the He-Ne laser modes are given. Moreover we present a novel, generic and non-invasive characterization method of the etalons to be used for the proposed HSRL. This feature allows highest accuracy in distinguishing the aerosol and molecular backscattered signals. © 2011 Elsevier B.V.	en
heal.journalName	Nuclear Physics B - Proceedings Supplements	en
dc.identifier.doi	10.1016/j.nuclphysbps.2011.04.026	en
dc.identifier.volume	215	en
dc.identifier.issue	1	en
dc.identifier.spage	265	en
dc.identifier.epage	268	en