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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, especially Muons
- Extremely powerful cosmic rays are raining down on us. No one knows where they come from. But with large-scale experiments, scientists around the world are determined to find out. Vox Jul 25, 2019
- Cosmic rays: particles from outer space Earth is subject to a constant bombardment of subatomic particles that can reach energies far higher than the largest machines. CERN
- "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 our Detectors are assembled
The Hardware
SiPM PCB
The SiPM photo sensor which detects the dim light generated inside the scintillation detector is mounted on a small SiPM board. Different numbers of SiPMs and read-out configurations can be realized through it's flexible design.
Preamplifier
The preamplifier is located in close vicinity to the 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 board's design is open source hardware and exhibits only commercially available off-the-shelf components which can be obtained from several distributors. With some soldering experience, the MuonPi HAT can be assembled utilizing a standard soldering equipment. A how-to guide and useful hints are available in the Assembly Guide.
The Software
The MuonPi software collection is entirely open source and available on github It consists of several components:
- muondetector-daemon The main control program running as a background system service on the RPi. The daemon configures, controls and supervises the components on the MuonPi HAT board, handles the comunication to the u-Blox chip and to the outside world via MQTT link and direct access socket, monitors system parameters, such as temperature, voltages, curent, rates etc., performs statistics collections, calculations and logging and much more. The daemon can be installed through the standard system software management tools (such as apt) from our package repository or compiled from the github source and is everything which is needed to operate a MuonPi detector.
- muondetector-gui A graphical user interface (GUI) program which can be launched on any computer in the same network as the MuonPi detector in order to monitor and adjust all operation parameters of the detector, if required. The GUI is available for download as binary package for several platforms (Raspbian, Ubuntu, Windows) or can be compiled from the current github master branch.
- muondetector-login A small command line helper tool to initially set up the MQTT telemetry link. The program will ask for the supplied MQTT credentials and stores them locally in encrypted form for continuous use.
- muondetector-cluster Allows the operation of a multi-detector cluster as an entity. The program is the cluster head or interface towards the server, searches for coincidences within the cluster and sends the combined coincidence events instead of the single event telegrams to the server. This tool is in development phase with more information about it's utilization to come in near future.
Setup and Operation of the Detector
Here you find a collection of HOW-TOs useful to set-up and operate a detector:
- Detector Surveillance through a Telegram Bot
The completed setup is fairly insensitive to the location where it will operate. Basic requirement is a good GPS signal, low humidity and obviously power and network connectivity. A stable temperature for the scintillator and preamp is desirable, as it affects the noise level of the setup. Muons will penetrate several meters of granite rock, so placing the detector in the basement leaves the muon measurements unaffected. However due to radon collection in basement rooms and potassium decay a slightly higher natural radioactive background can be observed.
In case there are problems with the set-up or operation of the detector, have a look in the Troubleshooting section.
Related Articles
News and articles about cosmic rays and similar projects.
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Admin Area
Useful resources for admins.
Users' Detectors Galery
About this Wiki
- How to edit? help for creators
- List of config variables
- MediaWiki-FAQ
- Mailing list of new MediaWiki version announcements
Sandbox page for testing/playing:
