The atmospheric monitoring system of the JEM-EUSO instrument

The JEM-EUSO Collaboration

doi:10.1007/s10686-014-9378-1

The atmospheric monitoring system of the JEM-EUSO instrument

The JEM-EUSO Collaboration

Research output: Contribution to journal › Article › peer-review

15 Scopus citations

Abstract

The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m.

Original language	English
Pages (from-to)	45-60
Number of pages	16
Journal	Experimental Astronomy
Volume	40
Issue number	1
DOIs	https://doi.org/10.1007/s10686-014-9378-1
State	Published - 1 Nov 2015
Externally published	Yes

Keywords

Atmospheric monitoring
IR camera
LIDAR
Ultra high energy cosmic rays

Access to Document

10.1007/s10686-014-9378-1

Cite this

@article{b10e1581b61f4e7c8aa081bca6fc2f81,

title = "The atmospheric monitoring system of the JEM-EUSO instrument",

abstract = "The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth{\textquoteright}s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m.",

keywords = "Atmospheric monitoring, IR camera, LIDAR, Ultra high energy cosmic rays",

author = "\{The JEM-EUSO Collaboration\} and Adams, \{J. H.\} and S. Ahmad and Albert, \{J. N.\} and D. Allard and L. Anchordoqui and V. Andreev and A. Anzalone and Y. Arai and K. Asano and \{Ave Pernas\}, M. and P. Baragatti and P. Barrillon and T. Batsch and J. Bayer and R. Bechini and T. Belenguer and R. Bellotti and K. Belov and Berlind, \{A. A.\} and M. Bertaina and Biermann, \{P. L.\} and S. Biktemerova and C. Blaksley and N. Blanc and J. B{\l}ȩcki and S. Blin-Bondil and J. Bl{\"u}mer and P. Bobik and M. Bogomilov and M. Bonamente and Briggs, \{M. S.\} and S. Briz and A. Bruno and F. Cafagna and D. Campana and Capdevielle, \{J. N.\} and R. Caruso and M. Casolino and C. Cassardo and G. Castellinic and C. Catalano and G. Catalano and A. Cellino and M. Chikawa and Christl, \{M. J.\} and D. Cline and V. Connaughton and L. Conti and G. Cordero and T. Kajino",

note = "Publisher Copyright: {\textcopyright} 2014, Springer Science+Business Media Dordrecht.",

year = "2015",

month = nov,

day = "1",

doi = "10.1007/s10686-014-9378-1",

language = "英语",

volume = "40",

pages = "45--60",

journal = "Experimental Astronomy",

issn = "0922-6435",

publisher = "Springer Netherlands",

number = "1",

}

TY - JOUR

T1 - The atmospheric monitoring system of the JEM-EUSO instrument

AU - The JEM-EUSO Collaboration

AU - Adams, J. H.

AU - Ahmad, S.

AU - Albert, J. N.

AU - Allard, D.

AU - Anchordoqui, L.

AU - Andreev, V.

AU - Anzalone, A.

AU - Arai, Y.

AU - Asano, K.

AU - Ave Pernas, M.

AU - Baragatti, P.

AU - Barrillon, P.

AU - Batsch, T.

AU - Bayer, J.

AU - Bechini, R.

AU - Belenguer, T.

AU - Bellotti, R.

AU - Belov, K.

AU - Berlind, A. A.

AU - Bertaina, M.

AU - Biermann, P. L.

AU - Biktemerova, S.

AU - Blaksley, C.

AU - Blanc, N.

AU - Błȩcki, J.

AU - Blin-Bondil, S.

AU - Blümer, J.

AU - Bobik, P.

AU - Bogomilov, M.

AU - Bonamente, M.

AU - Briggs, M. S.

AU - Briz, S.

AU - Bruno, A.

AU - Cafagna, F.

AU - Campana, D.

AU - Capdevielle, J. N.

AU - Caruso, R.

AU - Casolino, M.

AU - Cassardo, C.

AU - Castellinic, G.

AU - Catalano, C.

AU - Catalano, G.

AU - Cellino, A.

AU - Chikawa, M.

AU - Christl, M. J.

AU - Cline, D.

AU - Connaughton, V.

AU - Conti, L.

AU - Cordero, G.

AU - Kajino, T.

PY - 2015/11/1

Y1 - 2015/11/1

N2 - The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m.

AB - The JEM-EUSO telescope will detect Ultra-High Energy Cosmic Rays (UHECRs) from space, detecting the UV Fluorescence Light produced by Extensive Air Showers (EAS) induced by the interaction of the cosmic rays with the earth’s atmosphere. The capability to reconstruct the properties of the primary cosmic ray depends on the accurate measurement of the atmospheric conditions in the region of EAS development. The Atmospheric Monitoring (AM) system of JEM-EUSO will host a LIDAR, operating in the UV band, and an Infrared camera to monitor the cloud cover in the JEM-EUSO Field of View, in order to be sensitive to clouds with an optical depth τ ≥ 0.15 and to measure the cloud top altitude with an accuracy of 500 m and an altitude resolution of 500 m.

KW - Atmospheric monitoring

KW - IR camera

KW - LIDAR

KW - Ultra high energy cosmic rays

UR - https://www.scopus.com/pages/publications/84961711367

U2 - 10.1007/s10686-014-9378-1

DO - 10.1007/s10686-014-9378-1

M3 - 文章

AN - SCOPUS:84961711367

SN - 0922-6435

VL - 40

SP - 45

EP - 60

JO - Experimental Astronomy

JF - Experimental Astronomy

IS - 1

ER -

The atmospheric monitoring system of the JEM-EUSO instrument

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this