Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment

G. Agnetta; P. Assis; B. Biondo; P. Brogueira; A. Cappa; O. Catalano; J. Chauvin; G. D'Alí Staiti; M. Dattoli; M. C. Espirito-Santo; L. Fava; P. Galeotti; S. Giarrusso; G. Gugliotta; G. La Rosa; D. Lebrun; M. C. Maccarone; A. Mangano; L. Melo; S. Moreggia; M. Pimenta; F. Russo; O. Saavedra; A. Segreto; J. C. Silva; P. Stassi; B. Tomè; P. Vallania; C. Vigorito

doi:10.1016/j.nima.2006.09.102

Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment

G. Agnetta
, P. Assis
, B. Biondo
, P. Brogueira
, A. Cappa
, O. Catalano
, J. Chauvin
, G. D'Alí Staiti
, M. Dattoli
, M. C. Espirito-Santo
, L. Fava
, P. Galeotti
, S. Giarrusso
, G. Gugliotta
, G. La Rosa
, D. Lebrun
, M. C. Maccarone
, A. Mangano
, L. Melo
, S. Moreggia

M. Pimenta, F. Russo, O. Saavedra, A. Segreto, J. C. Silva, P. Stassi, B. Tomè, P. Vallania, C. Vigorito

INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
Lisboa
INFN Sezione di Catania
University of Turin
INFN Sezione di Torino
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
University of Palermo
INAF

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

The Uv Light Transmission and Reflection in the Atmosphere (ULTRA) experiment has been designed to provide quantitative measurements of the backscattered Cherenkov signal associated to the Extensive Air Showers (EAS) at the impact point on the Earth surface. The knowledge of such information will test the possibility to detect the diffused Cherenkov light spot from space within the Ultra high-energy cosmic ray observation. The Cherenkov signal is necessary to give an absolute reference for the track, allowing the measurement of the shower maximum and easing the separation between neutrino and hadronic showers. In this paper we discuss the experimental set-up with detailed information on the detection method; the in situ and laboratory calibrations; the simulation of the expected detector response and finally the preliminary results on the detector performance.

langue originale	Anglais
Pages (de - à)	22-35
Nombre de pages	14
journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	570
Numéro de publication	1
Les DOIs	https://doi.org/10.1016/j.nima.2006.09.102
état	Publié - 1 janv. 2007
Modification externe	Oui

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10.1016/j.nima.2006.09.102

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Agnetta, G., Assis, P., Biondo, B., Brogueira, P., Cappa, A., Catalano, O., Chauvin, J., D'Alí Staiti, G., Dattoli, M., Espirito-Santo, M. C., Fava, L., Galeotti, P., Giarrusso, S., Gugliotta, G., La Rosa, G., Lebrun, D., Maccarone, M. C., Mangano, A., Melo, L., ... Vigorito, C. (2007). Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 570(1), 22-35. https://doi.org/10.1016/j.nima.2006.09.102

@article{4849026e274e49259327c0b353793c77,

title = "Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment",

abstract = "The Uv Light Transmission and Reflection in the Atmosphere (ULTRA) experiment has been designed to provide quantitative measurements of the backscattered Cherenkov signal associated to the Extensive Air Showers (EAS) at the impact point on the Earth surface. The knowledge of such information will test the possibility to detect the diffused Cherenkov light spot from space within the Ultra high-energy cosmic ray observation. The Cherenkov signal is necessary to give an absolute reference for the track, allowing the measurement of the shower maximum and easing the separation between neutrino and hadronic showers. In this paper we discuss the experimental set-up with detailed information on the detection method; the in situ and laboratory calibrations; the simulation of the expected detector response and finally the preliminary results on the detector performance.",

keywords = "Cherenkov radiation, Cosmic ray detectors, Cosmic rays, Extensive air showers",

author = "G. Agnetta and P. Assis and B. Biondo and P. Brogueira and A. Cappa and O. Catalano and J. Chauvin and \{D'Al{\'i} Staiti\}, G. and M. Dattoli and Espirito-Santo, \{M. C.\} and L. Fava and P. Galeotti and S. Giarrusso and G. Gugliotta and \{La Rosa\}, G. and D. Lebrun and Maccarone, \{M. C.\} and A. Mangano and L. Melo and S. Moreggia and M. Pimenta and F. Russo and O. Saavedra and A. Segreto and Silva, \{J. C.\} and P. Stassi and B. Tom{\`e} and P. Vallania and C. Vigorito",

year = "2007",

month = jan,

day = "1",

doi = "10.1016/j.nima.2006.09.102",

language = "English",

volume = "570",

pages = "22--35",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

number = "1",

}

Agnetta, G, Assis, P, Biondo, B, Brogueira, P, Cappa, A, Catalano, O, Chauvin, J, D'Alí Staiti, G, Dattoli, M, Espirito-Santo, MC, Fava, L, Galeotti, P, Giarrusso, S, Gugliotta, G, La Rosa, G, Lebrun, D, Maccarone, MC, Mangano, A, Melo, L, Moreggia, S, Pimenta, M, Russo, F, Saavedra, O, Segreto, A, Silva, JC, Stassi, P, Tomè, B, Vallania, P & Vigorito, C 2007, 'Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, VOL. 570, Numéro 1, p. 22-35. https://doi.org/10.1016/j.nima.2006.09.102

Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment. / Agnetta, G.; Assis, P.; Biondo, B. et al.
Dans: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol 570, Numéro 1, 01.01.2007, p. 22-35.

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

TY - JOUR

T1 - Extensive air showers and diffused Cherenkov light detection

T2 - The ULTRA experiment

AU - Agnetta, G.

AU - Assis, P.

AU - Biondo, B.

AU - Brogueira, P.

AU - Cappa, A.

AU - Catalano, O.

AU - Chauvin, J.

AU - D'Alí Staiti, G.

AU - Dattoli, M.

AU - Espirito-Santo, M. C.

AU - Fava, L.

AU - Galeotti, P.

AU - Giarrusso, S.

AU - Gugliotta, G.

AU - La Rosa, G.

AU - Lebrun, D.

AU - Maccarone, M. C.

AU - Mangano, A.

AU - Melo, L.

AU - Moreggia, S.

AU - Pimenta, M.

AU - Russo, F.

AU - Saavedra, O.

AU - Segreto, A.

AU - Silva, J. C.

AU - Stassi, P.

AU - Tomè, B.

AU - Vallania, P.

AU - Vigorito, C.

PY - 2007/1/1

Y1 - 2007/1/1

N2 - The Uv Light Transmission and Reflection in the Atmosphere (ULTRA) experiment has been designed to provide quantitative measurements of the backscattered Cherenkov signal associated to the Extensive Air Showers (EAS) at the impact point on the Earth surface. The knowledge of such information will test the possibility to detect the diffused Cherenkov light spot from space within the Ultra high-energy cosmic ray observation. The Cherenkov signal is necessary to give an absolute reference for the track, allowing the measurement of the shower maximum and easing the separation between neutrino and hadronic showers. In this paper we discuss the experimental set-up with detailed information on the detection method; the in situ and laboratory calibrations; the simulation of the expected detector response and finally the preliminary results on the detector performance.

AB - The Uv Light Transmission and Reflection in the Atmosphere (ULTRA) experiment has been designed to provide quantitative measurements of the backscattered Cherenkov signal associated to the Extensive Air Showers (EAS) at the impact point on the Earth surface. The knowledge of such information will test the possibility to detect the diffused Cherenkov light spot from space within the Ultra high-energy cosmic ray observation. The Cherenkov signal is necessary to give an absolute reference for the track, allowing the measurement of the shower maximum and easing the separation between neutrino and hadronic showers. In this paper we discuss the experimental set-up with detailed information on the detection method; the in situ and laboratory calibrations; the simulation of the expected detector response and finally the preliminary results on the detector performance.

KW - Cherenkov radiation

KW - Cosmic ray detectors

KW - Cosmic rays

KW - Extensive air showers

UR - https://www.scopus.com/pages/publications/33845525774

U2 - 10.1016/j.nima.2006.09.102

DO - 10.1016/j.nima.2006.09.102

M3 - Article

AN - SCOPUS:33845525774

SN - 0168-9002

VL - 570

SP - 22

EP - 35

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 1

ER -

Extensive air showers and diffused Cherenkov light detection: The ULTRA experiment

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