Abstract

Mini-EUSO is part of the JEM-EUSO program and operates on board the International Space Station (ISS). It is a UV-telescope with single-photon counting capability looking at nighttime downwards to the Earth through a nadir-facing UV-transparent window. As part of the pre-flight tests, the Mini-EUSO engineering model, a telescope with 1/9 of the original focal surface and a lens of 2.5 cm diameter, has been built and tested. Tests of the Mini-EUSO engineering model have been made in laboratory and in open-sky conditions. Laboratory tests have been performed at the TurLab facility, located at the Physics Department of the University of Turin, equipped with a rotating tank containing different types of materials and light sources. In this way, the configuration for the observation of the Earth from space was emulated, including the Mini-EUSO trigger schemes. In addition to the qualification and calibration tests, the Mini-EUSO engineering model has also been used to evaluate the possibility of using a JEM-EUSO-type detector for applications such as observation of space debris. Furthermore, observations in open-sky conditions allowed the studies of natural light sources such as stars, meteors, planets, and artificial light sources such as airplanes, satellites reflecting the sunlight, and city lights. Most of these targets could be detected also with Mini-EUSO. In this paper, the tests in laboratory and in open-sky conditions are reported, as well as the obtained results. In addition, the contribution that such tests provided to foresee and improve the performance of Mini-EUSO on board the ISS is discussed.

Highlights

  • Mini-EUSO [1] is the first space-based mission of the JEM-EUSO (Joint Experiment Missions for Extreme Universe Space Observatory) program [2], installed inside the International Space Station (ISS)

  • When charged particles in extensive air showers induced by primary cosmic rays excite nitrogen molecules in the atmosphere, the molecular fluorescence transition leads to the isotropic light emission in the near-UV band (290-430 nm), which can be detected with highly sensitive telescopes at nighttime

  • The observations made with the Mini-EUSO EM offered an opportunity to test the prototype of the Mini-EUSO detector before it was launched and installed on the ISS in 2019

Read more

Summary

Introduction

Mini-EUSO [1] is the first space-based mission of the JEM-EUSO (Joint Experiment Missions for Extreme Universe Space Observatory) program [2], installed inside the International Space Station (ISS). The present configuration of Mini-EUSO on the ISS is not optimal for the detection of orbiting space debris, it is important to study the capability of the JEMEUSO-like telescopes [4] to detect and track them For their high temporal sampling rates, this type of telescopes are under consideration for the development of a system. A few meteor candidates, and a large-scale space debris (a rocket body) have been observed from the Astrophysical Observatory, where the sky conditions allowed observation of faint sources, as well as artificial lights from nearby cities. These measurements and related results are presented and discussed in this paper

Mini-EUSO
The Mini-EUSO EM
Tests at TurLab
The Mini-EUSO EM at TurLab
Tests on the L2 trigger and D3 continuous data acquisition
Measurements for space debris studies
Mini-EUSO EM at the Astrophysical Observatory of Turin
Stars and planets
Meteors
Night sky brightness
Rocket of a telecommunication satellite and airplane
Comparing Mini-EUSO EM tests with preliminary Mini-EUSO data
Conclusions
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call