Hybrid Active-Passive Galactic Cosmic Ray Simulator: experimental implementation and microdosimetric characterization
Enrico Pierobon, Luca Lunati, Tim Wagner, Marco Durante, Christoph Schuy
TL;DR
The paper addresses the challenge of ground-based Galactic Cosmic Ray (GCR) studies by introducing a European hybrid active-passive GCR simulator that reproduces a space-like radiation field through six sequential configurations weighted to match a 1 AU, solar-minimum environment after aluminum shielding. The approach combines an energy-switching primary beam, passive mesh/complex/slab modulators, TEPC microdosimetry, and Geant4 Monte Carlo validation to characterize the resulting field and extract quality factors. Key contributions include experimental microdosimetric spectra for each configuration, a weighted total spectrum that approximates a GCR field, and validation of the designed quality factor against measurements and space data, supporting the simulator’s relevance for electronics and biology research. The European facility provides a path to bridge physical radiation description with biological outcomes, with planned accessibility in 2026 to enable comprehensive GCR studies on Earth.
Abstract
Space radiation is one of the major obstacles to space exploration. If not mitigated, radiation can interact both with biological and electronic systems, inducing damage and posing significant risk to space missions. Countermeasures can only be studied effectively with ground-based accelerators that act as a proxy for space radiation. Following an in-silico design and optimization process we have developed a galactic cosmic ray (GCR) simulator using a hybrid active-passive methodology. In this approach, the primary beam energy is actively switched and the beam interacts with specifically designed passive modulators. In this paper, we present the implementation of such a GCR simulator and its experimental microdosimetric characterization. Measuring the GCR field is of paramount importance, both before providing it to the user as a validated radiation field and for achieving the best possible radiation description. The issue is addressed in this paper by using a tissue equivalent proportional counter to measure radiation quality and by comparing experimental measurements with Monte Carlo simulations. In conclusion, we will demonstrate the GCR simulator's capability to reproduce a GCR field.
