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In order to determine the non-uniformity of the CsI light throughout the volume of the modules, a reconstruction technique similar to that used in nuclear medicine imaging is needed. In the case of the pion beta tomography, the directions and the pathlengths of the cosmic muons in the CsI modules are obtained from the drift chambers. If the volume of a crystal is subdivided into elementary cells, a cosmic muon traversing the module will deposit energies in the cells which lie along the particle path. The energy deposited depends on the segments of the particle's trajectory in the cells. A geometrical algorithm has been designed to trace the particle's trajectory through the crystals, and to find the number and the actual pathlength in each of the cells traversed. However for a given cosmic ray, only the total sum of the light outputs in the cells traversed is known from the CsI ADC. The reconstruction method allows the determination of the light per pathlength in the elementary cells of the CsI module, and enables the study of the non-uniformity of the generation and collection of the CsI light in the volume of the crystals.

The principle of the reconstruction technique consists of taking initial guesses at the lights per pathlengths in the elementary cells.

Table: Some parameters of the six crystal measured with the tomography system. The non-uniformity in the fourth column is affected by the light generated close to the PMT --- solid angle effect. When the non-uniformity functions are weighted with the energies of the showers initiated by 70 MeV 's incident along the crystal axes, the detector responses are more uniform. The temperature coefficients were calculated assuming a linear dependence of the light output on the temperature. For the fast and the total components, the ADC integration times were 100 ns and respectively.

Then new guesses are taken based on the discrepancies between the calculated light outputs (from the previous trial) and the measured ones. An iterative process is then initiated until the process converges. Four of the existing reconstruction techniques [Bud-74] have tested for their convergences and their abilities to handle noisy data. The four methods tested are the additive and multiplicative versions of the algebraic reconstruction technique (ART), the simultaneous iterative reconstruction (SIRT) and the least-square iterative approach. These techniques have been tested with a sample of simulated data consisting of a signal riding on an isotropic background. In 500 iterations, the SIRT reconstructed the data, especially the signal as a region of intensity above the uniform backgroundgif.

Figure: The light non-uniformity obtained from the reconstruction procedure for one CsI module (serial # S011) in the box. 28000 events with multiple scattering angles were considered for the reconstruction. The volume of the elementary cells was . Three orthogonal cuts through the crystal are shown here, and the text histograms display the average light outputs (MeV) in the cells. The average energy deposited in the CsI by the cosmic muons is , while the most probable energy loss is 5.92 MeV/cm.

Some results of the reconstruction are shown in figure gif for one of the modules in the box. Figure gif shows the light non-uniformity along the axis of a set of six crystals in the box, and some results of the tomography are summarized in table gif.

Figure: The light collection non-uniformity along the axes of six crystals measured with the tomography system. The cosmic rays with polar angles in axial strips of were analyzed. The result of the reconstruction technique summed over the cells which satisfy the same cuts is shown as the dashed line for the module S011.

In conclusion the tomography apparatus is under stable operation and a reconstruction technique has been worked out to examine each of the calorimeter modules. Up to six crystals can be inserted in the apparatus at a time. It takes about a week of data taking to collect enough statistics for one set of crystals in the box. During that period another batch of six modules are prepared and ready to be set-up for the tomography. As stated previously, tomography data have been taken for forty-seven crystals to date. The results presented here are likely to be improved upon with a refinement of the reconstruction technique and the analysis of the data. The goal is to build the calorimeter using modules with non-uniformity less than

(section 7.6). The crystals of that quality are being selected through the tomography method described here. For the responses of an array of twelve calorimeter modules to monoenergetic beam of 's, a non-uniformity of --- this was inferred from the surface treatment studies for a wrapping method consisting of three layers of teflon and black paper at the front face (see figure 8.4) --- has been used to obtain excellent agreement between data and simulation (section 8.1.3). The tomography method reveals the non-uniformity throughout the volumes of the modules, and consequently will render the simulation of the experiment even more realistic.

next up previous contents
Next: Calorimeter Response to Up: Cosmic Ray Tomography Previous: Calibration of the

Bernward Krause
Mon Jan 15 14:57:06 MET 1996