The CALorimetric Electron Telescope (CALET) mission is proposed for the observation of high energy cosmic rays and gamma radiation for the JEM-EF attached payload on the International Space Station. The instrument, equipped with an imaging calorimeter of scintillating fibers (IMC) and a total absorption BGO calorimeter (TASC), is optimized for the measurement of cosmic ray electrons in the TeV energy range with the exciting possibility to identify individual nearby sources. The large collection power of CALET also allows for precision studies of the elemental composition of charged cosmic rays and of their spectral features. The charge identification of the incoming particle is performed by a two-layered array of pixelated silicon sensors, covering a seamless sensitive area of about 0.8 m^2, placed on top of the instrument. An innovative integrated design of the array and its front-end electronics will be presented.
Marrocchesi, P.S., Avanzini, C., Bagliesi, M.G., Basti, A., Batkov, K., Bigongiari, G., et al. (2008). Conceptual design of a charge identifier array for cosmic ray composition measurements in CALET. In Proceedings of the 30th International Cosmic Ray Conference (pp.301-304). MERIDA : Universidad Nacional Autónoma de México.
Conceptual design of a charge identifier array for cosmic ray composition measurements in CALET
MARROCCHESI P. S.;BATKOV K.;BIGONGIARI G.;CALDARONE A.;CECCHI R.;MAESTRO P.;MILLUCCI V.;ZEI R.
2008-01-01
Abstract
The CALorimetric Electron Telescope (CALET) mission is proposed for the observation of high energy cosmic rays and gamma radiation for the JEM-EF attached payload on the International Space Station. The instrument, equipped with an imaging calorimeter of scintillating fibers (IMC) and a total absorption BGO calorimeter (TASC), is optimized for the measurement of cosmic ray electrons in the TeV energy range with the exciting possibility to identify individual nearby sources. The large collection power of CALET also allows for precision studies of the elemental composition of charged cosmic rays and of their spectral features. The charge identification of the incoming particle is performed by a two-layered array of pixelated silicon sensors, covering a seamless sensitive area of about 0.8 m^2, placed on top of the instrument. An innovative integrated design of the array and its front-end electronics will be presented.File | Dimensione | Formato | |
---|---|---|---|
icrc141.pdf
non disponibili
Tipologia:
Post-print
Licenza:
NON PUBBLICO - Accesso privato/ristretto
Dimensione
140.72 kB
Formato
Adobe PDF
|
140.72 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
https://hdl.handle.net/11365/30229