6–11 Jun 2010
Village de Vacances de Lamoura
Europe/Zurich timezone

Session

Working Group - Synergies in Data Acquisition

8 Jun 2010, 17:20
Village de Vacances de Lamoura

Village de Vacances de Lamoura

39310 Lamoura France

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  1. Haik Simon
    08/06/2010, 17:20
    working group on synergies in electronics and data acquisition
    oral with financial aid
    The experimental program at FAIR requires a smooth transition from existing experiments as well as integrating a variety of old and new detector systems from different collaborations world-wide. We follow a flexible scheme where minimal functionalities of an associated electronics, readout and control are defined in order to make these complex systems work together. In my talk I will present...
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  2. Mr H.J. WOERTCHE (INCAS)
    08/06/2010, 17:40
    working group on synergies in electronics and data acquisition
    invited
    I will present the organizational structure and the research program of INCAS3, a starting research institute focusing on the development of advanced sensor technology. INCAS3 is co-financed by the Northern-Netherlands Provinces, the European Union, European Fund for Regional Development and the Dutch Ministry of Economic affaires. The mission of INCAS3 is to translate business and...
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  3. Michel TRIPON (GANIL)
    08/06/2010, 18:10
    working group on synergies in electronics and data acquisition
    invited
    Along with the implementation of SPIRAL2 , the second generation of RIB accelerator of the GANIL laboratory , have emerged projects of new detectors and instrumentations which comply with new constraints brought by high intensities RIB, such as higher counting rates, higher number of channels, higher data readout rate, fast link connections between DAQ instrumentations, experimental cave...
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  4. Maurizio BINI (INFN Firenze)
    08/06/2010, 18:30
    working group on synergies in electronics and data acquisition
    invited
    The development of the Fazia FEE design will be presented, concerning the main problems that have been attacked. In order to minimize noise and signal distortion the solution of the digitizer back-to-back the preamplifier inside the vacuum chamber has been adopted. With the digitizing ADCs (6 for each telescope composed of two Silicon detectors of 300 and 500 micron followed by a CsI) each...
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  5. 08/06/2010, 18:50
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