Real-time systems, acquisition electronics and microelectronics (STREAM)

Real-time systems, acquisition electronics and microelectronics (STREAM)

STREAM: Laboratoire des Systèmes Temps Réel, Electronique d’Acquisition et Microélectronique designs and produces analog, digital and programmable electronics for the detection instruments used in experiments in the Institute’s various fields of research

The laboratory brings together 14 permanent and 6 non-permanent staff in the following fields: analog and mixed analog/digital microelectronics, associated support for characterization, chip bonding and production testing of special-purpose integrated circuits (ASICs), data acquisition system architecture, analog and/or digital electronic board design, firmware programming of field-programmable logic circuits (FPGAs) and embedded real-time system computing.

The STREAM laboratory works in synergy with the Institute’s physics departments and other Sédi laboratories to make significant contributions to leading scientific experiments.

The trajectograph acquisition system for the Clas12 nuclear physics experiment is an example of this combination of skills: the DREAM chip, designed in the STREAM laboratory and based on know-how in low-noise analog microelectronics and analog memories, is the basic building block of the FEU front-end boards, co-developed with Liseta. These cards read cylindrical Micromegas detectors developed at SEDI. This reading system, which will ultimately comprise 20,000 channels, is currently being delivered and installed at Jefferson Lab (USA). On the Franco-Chinese SVOM space mission, STREAM and Lilas laboratories are sharing development of the firmware and on-board software for the satellite’s Scientific and Technical Management Unit (UGTS). The STREAM laboratory also designed and produced the flight ASICs for the ECLAIRs wide-field telescope, a key element of SVOM’s payload. Still for space applications, the STREAM laboratory’s expertise in low-noise radiation-hardened microelectronics enabled it to develop and produce, in collaboration with the astrophysics department, the “Caliste” hybrid micro-gamma camera for the Solar Orbiter satellite.

The DREAM ASIC: 700,000 transistors, 1/2 cm2. Each of the 64 channels converts the detector signal, filters it and stores its shape in 512 analog memory points.

The laboratory’s other main current projects concern Phase 1 of the Large Hadron Collider (LHC) experimental enhancement program at CERN, with a microelectronics contribution to the monolithic pixelated silicon detectors of the ALICE Muon Forward Tracker, and responsibility for the design and production of the 600 or so SOLAR front-end boards for the Bras-Dimuon. In the ATLAS experiment, the STREAM and LISETA laboratories share responsibility with American partners for the design and production of the ~150 high-performance, radiation-hardened “LTDB” digitizing cards.

One of the laboratory’s R&D activities concerns cryogenic microelectronics and the design of superconducting filaments for reading infrared or X-ray bolometer arrays for astrophysics applications.

The laboratory is also anticipating the ramp-up to Phase 2 of the LHC experimental enhancement program by developing high-voltage CMOS pixel detectors for the ATLAS internal trajectograph. Similarly, the future front-end ASIC for the central part of the CMS electromagnetic calorimeter is currently being designed in the laboratory.

Prototype of the Liquid argon calorimeter Trigger Digitizer Board (LTDB). This radiation-hardened board is a 320-channel, 12-bit, 40 MHz amplifier-digitizer with optical outputs (192 Gbit/s total gross data rate). The final model will integrate over 10,000 components on a 24-layer printed circuit board measuring 41 cm x 50 cm. One hundred and fifty units will be used in the ATLAS experiment.

Projets

  • ALICE

    ALICE

    The ALICE experiment is devoted to the study of nuclear matter under extreme conditions of temperature and density. It is specially designed to test the fundamental theory of the strong interaction,…

  • ATHENA

    ATHENA

    Un satellite pour l’étude del’univers chaud et énergétique. Lancement prévu pour 2031. A satellite to study hot and energetic universe to be launched in 2031.

  • BAO

    BAO

    Most of the content of the Universe, about 70%, is dominated by an energetic component that is neither matter nor radiation: dark energy. This mysterious component, first observed in 1998 with…

  • CLAS12

    CLAS12

    Deeply Virtual Compton Scattering experiment at Jefferson Lab Hall B , with CLAS12, large acceptance spectrometer. Goals: Theoretical concepts asGeneralized Parton Distributions (GPD), enable to…

  • Edelweiss

    Edelweiss

    Objectives The goal of Edelweiss is to detect the dark matter of our Galaxy through its interactions in detectors operated in underground laboratory. The EROS experiment, searching for massive…

  • HESS

    HESS

    H.E.S.S. Exploring the High Energy gamma ray sky H.E.S.S stands for “High Energy Stereoscopic System”. This telescope system been designed and built by a large international collaboration which…

  • MEGACAM

    MEGACAM

    Caméra installée au foyer du télescope de 3,6m de diamètre du CFHT. Camera installed on the 3,6m diameter telescope of the CFHT.

  • Solar Orbiter

    Solar Orbiter

    The objective of the Solar Orbiter mission is to understand the Sun’s influence on the heliosphere (its magnetic cocoon), in order to understand how our star influences our solar system.

  • SVOM

    SVOM

    A mission dedicated to the study of gamma ray bursts The SVOM Mission (Space based multi-band astronomical Variable Objects Monitor) is a chinese and french project dedicated to the detection and…

  • T2K

    T2K

    T2K (Tokai to Kamioka) is the world leading experiment dedicated to the study of neutrino oscillations over a long distance using µ-neutrino and µ-anti-neutrino beams. Neutrinos exist in three…

Thèses

Publications