Channeltron Detector Readout ASIC in 0.35µm HV CMOS for Cold Solar Wind Analysis

King Wah Wong (1) , Olivier Daniel Bernal (2) , Antoine Cara (1) , Andrei Fedorov (1) , Rituparna Baruah (1) , Romain Mathon (1) , Carine Amoros (1) , Hélène Tap (2) , Benoit Lavraud (1)

1 IRAP - Institut de recherche en astrophysique et planétologie
2 LAAS-OSE - Équipe Optoélectronique pour les Systèmes Embarqués

Low-power analog front-end circuits for channeltron detectors (or Channel Electron Multiplier: CEMs) have been fabricated in 0.35-μm CMOS technology to characterize low energy solar wind particles. They have been designed to readout signals for incident charges ranging from 50 fC to 20 pC. Each front end circuit consists of a charge preamplifier, an amplifier, a discriminator, a monostable circuit and a LVDS. Requirement on the complete front end is to consume less than 6.5 mW/channel for a maximum event detecting rate of 40 MHz.

Domaines: Micro et nanotechnologies/Microélectronique

King Wah Wong, Olivier Daniel Bernal, Antoine Cara, Andrei Fedorov, Rituparna Baruah, et al.. Channeltron Detector Readout ASIC in 0.35µm HV CMOS for Cold Solar Wind Analysis. International Workshop on Analogue and Mixed-Signal Integrated Circuits for Space Applications (AMICSA 2018), Jun 2018, Louvain, Belgium. ⟨hal-01985290⟩