The existance of high energy particles with energies >1020 eV in the space is a basic problem in fundermental physics, because it means a violation of the GZK theoretical limitation. JEM-EUSO will try to detect such high energy particles in the space by the oprical fluorescence from the high energy paticles incident to the atmosphere. For caliblation of the optical background an atmospheric monitoring system consisting of a spaceborne lidar with an ultraviolet pulsed laser and an IR camera will be used. The IR camera takes images at suitable time intervals, monitoring the cloud cover in the whole field of view (FoV) of the telescope. Moreover stereo images are also taken to retrieve pixel by pixel the height of the cloud-top. The ultraviolet lidar measures the height of surface of clouds with the 30 m resolution. From these measuremnts we obtain a 3 dimentional map of clouds. The laser specifications are 20mJ/pulses at 355nm 20Hz rate, single longitudinal mode, and M 2<1 with conduction cooling.

Wada, S., Ebisuzaki, T., Ogawa, T., Sato, M., Peter, T., Mitev, V., et al. (2009). Potential of the atmospheric monitoring system of JEM-EUSO mission. In 31st International Cosmic Ray Conference, ICRC 2009. Lodz : University of Lodz.

Potential of the atmospheric monitoring system of JEM-EUSO mission

TEGOLO, Domenico;
2009-01-01

Abstract

The existance of high energy particles with energies >1020 eV in the space is a basic problem in fundermental physics, because it means a violation of the GZK theoretical limitation. JEM-EUSO will try to detect such high energy particles in the space by the oprical fluorescence from the high energy paticles incident to the atmosphere. For caliblation of the optical background an atmospheric monitoring system consisting of a spaceborne lidar with an ultraviolet pulsed laser and an IR camera will be used. The IR camera takes images at suitable time intervals, monitoring the cloud cover in the whole field of view (FoV) of the telescope. Moreover stereo images are also taken to retrieve pixel by pixel the height of the cloud-top. The ultraviolet lidar measures the height of surface of clouds with the 30 m resolution. From these measuremnts we obtain a 3 dimentional map of clouds. The laser specifications are 20mJ/pulses at 355nm 20Hz rate, single longitudinal mode, and M 2<1 with conduction cooling.
2009
31st International Cosmic Ray Conference, ICRC 2009
Lodz, Poland
7 July 2009 through 15 July 2009;
Code 104675
2009
4
A stampa
Wada, S., Ebisuzaki, T., Ogawa, T., Sato, M., Peter, T., Mitev, V., et al. (2009). Potential of the atmospheric monitoring system of JEM-EUSO mission. In 31st International Cosmic Ray Conference, ICRC 2009. Lodz : University of Lodz.
Proceedings (atti dei congressi)
Wada, S.; Ebisuzaki, T.; Ogawa, T.; Sato, M.; Peter, T.; Mitev, V.; Matthey, R.; Anzalone, A.; Isgrò, F.; Tegolo, D.; Colombo, E.; Morales de los Rios, J.; Rodriguez Frias, M.; Il, P.; Shinwoo, N.; Jae, P.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/226393
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