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Conference paper

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

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University of Bergen, Department of Physics and Technology, Norway1

Technical University of Denmark, National Space Institute, Copenhagen, Denmark2

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.

Language: English
Year: 2012
Pages: 2124-2127
Proceedings: 2012 IEEE International Instrumentation and Measurement Technology Conference (I2MTC)
ISBN: 1457717719 , 1457717727 , 1457717735 , 9781457717710 , 9781457717727 and 9781457717734
ISSN: 10915281
Types: Conference paper
DOI: 10.1109/I2MTC.2012.6229186

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