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== [[preamp|Preamplifier]] == | == [[preamp|Preamplifier]] == | ||
| − | The preamp is located in close vicinity | + | The preamp is located in close vicinity to the [[sipm_board|SiPM photodetector board] and amplifies the weak signals for transmission to the [[mounpi_board|MuonPi]] board, where they are further processed and evaluated. |
== The MuonPi-Board == | == The MuonPi-Board == | ||
Revision as of 15:29, 5 April 2020
Contents
The MuonPi Cosmic Detector Project
The MuonPi Project is a RaspberryPi-based system using an inexpensive plastic scintillator + SiPM photo sensor to detect muons from cosmic air showers with a time-stamping accuracy of several tens of nanoseconds utilizing the u-blox NEO-M8N GNSS module's "timemark" feature.
Learn about cosmic radiation
- Get started with Cosmic Rays
- "Kosmische Strahlung" Podcast (in German) on weltderphysik.de
- "Der kosmischen Strahlung auf der Spur" article (in German) on weltderphysik.de
- "Kosmische Teilchen mit extragalaktischem Ursprung" article (in German) on weltderphysik.de
Learn about the detectors
- Basics of Scintillators
- Find out about Silicon photomultipliers
- How the MuonPi detectors are assembled
The Hardware
SiPM PCB
Preamplifier
The preamp is located in close vicinity to the [[sipm_board|SiPM photodetector board] and amplifies the weak signals for transmission to the MuonPi board, where they are further processed and evaluated.
The MuonPi-Board
The main signal processing, voltage generation and parameter monitoring and adjustment is done on the Raspberry Pi plug-on MuonPi Board.
The Software
About this Wiki
- How to edit? help for creators
