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A framework designed to simulate the signals produced by the secondary particles emerging from the interaction of the flux of primary cosmic ray with the atmosphere. These signals are simulated for any particle detector located at any place (latitude, longitude and altitude), including the real-time atmospheric, geomagnetic and detector conditions.
A vastly configurable and flexible geomagnetic observatory firmware for the Raspberry Pi Pico (RP2040). Currently supports a variety of sensors that output an analog signal or square wave (eg. FGM3-Plus/Pro). It reads, processes, displays and logs data, lets you configure settings/calibrations at runtime using an intuitive and powerful UI and more.