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DRAFT<br />

extracted beams. Its use for the <strong>Super</strong>-FRS is limited to intensities up to about 10 10-11 particles/spill<br />

to avoid damaging of the detector.<br />

Figure 2.4.86: Layout of the SEETRAM counter. It consists of titanium foils (#1) with 10 µm thickness<br />

sandwiched between two aluminium foils of 14 µm thickness each (#2 and #3). Each foil has a diameter of<br />

11.5 cm. They are mounted perpendicular to the beam axis. The outer foils are connected to a voltage of<br />

+80 V. They and their supporting aluminium rings form the detector housing. The middle foil is supported by<br />

two Teflon rings and is insulated against other parts of the detector. The foils are curved in order to reduce<br />

the sensitivity to mechanical vibration of the beam line. Secondary electrons emitted from the middle foil are<br />

collected by the two outer foils. The created current in the middle foil is measured by a current digitizer<br />

(CD1010 developed at GSI).<br />

In order to calibrate the current measurement up to now the calibration proceeds via two steps: first<br />

a scintillator detector is used in counting mode; second an ionization chamber takes over in order to<br />

calibrate the SEETRAM detector. For the <strong>Super</strong>-FRS we will benefit from the high counting rates<br />

that can be taken by a diamond detector (10 x 10 cm², PC-CVC-DD (AG)) and thus be able to leave<br />

out the ionization chamber. Thus we will be able to reduce the setup and calibration phase for the<br />

experiments. The diamond detector here can also be used at reduced rates of 10 9...10 /spill – as has<br />

been done already for the SIS18 – to analyze the spill structure after slow extraction from the<br />

different SIS rings.<br />

(ii) For the entrance of the main separator a SEETRAM counter and a diamond detector are<br />

planned to be used for the luminosity measurements. The diamond counter can be used (as shown<br />

in section 2.4.6.5) also as start counter for a time-of-flight measurement. The expected spot size is<br />

here about (2 x 3) mm² as given by the magnification (Mx = 2, My = 1.5) of the Pre-<strong>Separator</strong> optics.<br />

With rates up to 10 9 /s uranium ions, this is just at the limit of what can be counted using a<br />

PC-CVD-DD. One may consider using single crystal material here. The recent available<br />

SC-CVD-D material is presently investigated by NoRHDia [34]. The charge collection efficiency<br />

of SC-CVD-D detectors amount to almost 100 %, and the signal amplitudes are uniform over the<br />

detector area, which is not the case for PC-CVC-DD. However, due to much lower concentration<br />

of traps the detectors behave as fast drift chambers. Therefore, the count rate capability is lower<br />

and only 50 MHz are manageable. Instead of single particle counting one should investigate the<br />

89

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