NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Charge Resolution of the Silicon Matrix of the ATIC ExperimentATIC (Advanced Thin Ionization Calorimeter) is a balloon borne experiment designed to measure the cosmic ray composition for elements from hydrogen to iron and their energy spectra from approx.50 GeV to near 100 TeV. It consists of a Si-matrix detector to determine the charge of a CRT particle, a scintillator hodoscope for tracking, carbon interaction targets and a fully active BGO calorimeter. ATIC had its first flight from McMurdo, Antarctica from 28/12/2000 to 13/01/2001. The ATIC flight collected approximately 25 million events. The silicon matrix of the ATIC spectrometer is designed to resolve individual elements from proton to iron. To provide this resolution careful calibration of each pixel of the silicon matrix is required. Firstly, for each electronic channel of the matrix the pedestal value was subtracted taking into account its drift during the flight. The muon calibration made before the flight was used then to convert electric signals (in ADC channel number) to energy deposits in each pixel. However, the preflight muon calibration was not accurate enough for the purpose, because of lack of statistics in each pixel. To improve charge resolution the correction was done for the position of Helium peak in each pixel during the flight . The other way to set electric signals in electronics channels of the Si-matrix to one scale was correction for electric channel gains accurately measured in laboratory. In these measurements it was found that small different nonlinearities for different channels are present in the region of charge Z > 20. The correction for these non-linearities was not done yet. In linear approximation the method provides practically the same resolution as muon calibration plus He-peak correction. For searching a pixel with the signal of primary particle an indication from the cascade in the calorimeter was used. For this purpose a trajectory was reconstructed using weight centers of energy deposits in BGO layers. The point of intersection of this trajectory with Si-matrix and its RMS was determined. The pixel with maximal signal in 3sigma region was taken as sought. The signal in this pixel was corrected by trajectory zenith angle. The preliminary results on charge resolution of the Si-matrix in the range from protons to iron are presented.
Document ID
20020050658
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Zatsepin, V. I.
(Moscow State Univ. Russia)
Adams, J. H., Jr.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Ahn, H. S.
(Maryland Univ. United States)
Bashindzhagyan, G. L.
(Moscow State Univ. Russia)
Batkov, K. E.
(Moscow State Univ. Russia)
Case, G.
(Louisiana State Univ. United States)
Christl, M.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Ganel, O.
(Maryland Univ. United States)
Fazely, A. R.
(Southern Univ. United States)
Ganel, O.
(Maryland Univ. United States)
Six, N. Frank
Date Acquired
August 20, 2013
Publication Date
January 1, 2002
Subject Category
Instrumentation And Photography
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Available Downloads

There are no available downloads for this record.
No Preview Available