BGO front-end electronics and signal processing in the MXGS instrument for the ASIM mission

Publication: Research - peer-reviewArticle in proceedings – Annual report year: 2012

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DOI

  • Author: Skogseide, Yngve, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Cenkeramaddi, Linga Reddy, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Genov, Georgi, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Njoten, Kare, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Rostad, Maja Elise, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Solberg, Arne, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Stadsnes, Johan, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Ullaland, Kjetil, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Ostgaard, Nikolai, Norway

    Department of Physics and Technology, University of Bergen, Norway

  • Author: Budtz-Jørgensen, Carl

    Astrophysics, National Space Institute, Technical University of Denmark, Elektrovej, 2800, Kgs. Lyngby, Denmark

  • Author: Kuvvetli, Irfan

    Astrophysics, National Space Institute, Technical University of Denmark, Elektrovej, 2800, Kgs. Lyngby, Denmark

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This paper presents the Bismuth Germanate Oxide (BGO) front-end electronics design and signal processing in Modular X- and Gamma ray sensor (MXGS) instrument onboard the Atmosphere Space Interaction Monitor (ASIM) mission, funded by the European Space Agency. University of Bergen is responsible for the design and development of the detector layers and readout electronics for the MXGS instrument. The principal objective of the instrument is to detect Terrestrial Gamma ray Flashes (TGFs), which are related to thunderstorm activity. The digital pulse processing scheme used in the MXGS BGO detector gives it a significantly higher rate capability than what has been achieved in other instruments used in the study of terrestrial gamma flashes. The front-end electronics for the BGO detector layer in MXGS system also uses fewer components compared to conventional analog front-ends for BGO detectors, thereby increasing its reliability and projected lifetime in the harsh space environment. The MXGS instrument is expected to see about 1000 TGFs in a time period of one year.
Original languageEnglish
TitleProceedings of IEEE Instrumentation/Measurement Technology Conference (I2MTC)
Number of pages4
PublisherIEEE
Publication date2012
Pages2124-2127
ISBN (print)9781457717734
DOIs
StatePublished

Conference

ConferenceIEEE International Instrumentation and Measurement Technology Conference (I2MTC)
CountryAustria
CityGratz
Period13/05/1216/05/12
Internet addresshttp://imtc2012.ieee-ims.org/
CitationsWeb of Science® Times Cited: No match on DOI

Keywords

  • Gamma ray detector, X-ray detector, Radiation, Imaging, BGO detector, International Space Station, MXGS instrument, ASIM mission
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