Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework
arXiv:2311.12656 · doi:10.1140/epjc/s10052-023-12090-w
Abstract
JEM--EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. All instruments are based on a wide-field-of-view telescope, which operates in the near-UV range, designed to detect the fluorescence light emitted by extensive air showers in the atmosphere. We describe the simulation software ESAFin the framework of the JEM--EUSO program and explain the physical assumptions used. We present here the implementation of the JEM--EUSO, POEMMA, K--EUSO, TUS, Mini--EUSO, EUSO--SPB1 and EUSO--TA configurations in ESAF. For the first time ESAF simulation outputs are compared with experimental data.
References in corpus (27)
- The Pierre Auger Cosmic Ray Observatory
- Detection of a Cosmic Ray with Measured Energy Well Beyond the Expected Spectral Cutoff due to Cosmic Microwave Radiation
- The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment
- Measurement of the cosmic-ray energy spectrum above eV using the Pierre Auger Observatory
- The Offline Software Framework of the Pierre Auger Observatory
- Measurement of the cosmic ray energy spectrum with IceTop-73
- Depth of Ultra High Energy Cosmic Ray Induced Air Shower Maxima Measured by the Telescope Array Black Rock and Long Ridge FADC Fluorescence Detectors and Surface Array in Hybrid Mode
- The Jem-Euso Mission
- An evaluation of the exposure in nadir observation of the JEM-EUSO mission
- New measurement on photon yields from air and the application to the energy estimation of primary cosmic rays
- The TUS detector of extreme energy cosmic rays on board the Lomonosov satellite
- First Results of Fast One-dimensional Hybrid Simulation of EAS Using CONEX
- Observing the Ultrahigh Energy Universe with OWL Eyes
- ESAF: Full Simulation of Space-Based Extensive Air Showers Detectors
- Mini-EUSO mission to study Earth UV emissions on board the ISS
- Simulation of Ultra-High Energy Photon Propagation in the Geomagnetic Field
- Mini-EUSO: A high resolution detector for the study of terrestrial and cosmic UV emission from the International Space Station
- The integration and testing of the Mini-EUSO multi-level trigger system
- Observation of night-time emissions of the Earth in the near UV range from the International Space Station with the Mini-EUSO detector
- EUSO-SPB1 Mission and Science
- Performance and science reach of POEMMA for ultrahigh-energy particles
- An extensive-air-shower-like event registered with the TUS orbital detector
- Overview and First Results of EUSO-SPB2
- First observations of speed of light tracks by a fluorescence detector looking down on the atmosphere
- Development of a cosmic ray oriented trigger for the fluorescence telescope on EUSO-SPB2
- Kinematics reconstruction of the EAS-like events registered by the TUS detector
- Simulations studies for the Mini-EUSO detector