Mini-EUSO mission to study Earth UV emissions on board the ISS

Autor: E. Parizot, G. Valentini, Francesca Capel, M. Ricci, P. Picozza, A. Djakonow, M. Przybylak, A. Zuccaro-Marchi, M. Traïche, A. Franceschi, F. Cafagna, B. A. Khrenov, F. Fenu, C. de la Taille, Toshikazu Ebisuzaki, Hitoshi Ohmori, Satoshi Wada, P. Gorodetzky, M. Crisconio, Angela V. Olinto, Lech Wiktor Piotrowski, Marco Mignone, M. E. Bertaina, S. Turriziani, W. Marszał, G. Cotto, L. Marcelli, J. Szabelski, I. V. Yashin, H. Kasuga, Naoto Sakaki, Enzo Reali, Kenji Shinozaki, S. Kochepasov, S. Bacholle, A. Haungs, V. D. Kuznetsov, S. Blin-Bondil, Marco Casolino, Z. Plebaniak, Mikhail Panasyuk, I. Churilo, P. Barrillon, G. Prévôt, Pavel Klimov, A. V. Belov, A. Poroshin, L. R. Wiencke, G. Mascetti, G. Osteria, Y. Takizawa, H. Miyamoto, M. Porfilio, C. Blaksley, T. Napolitano, G. Cambiè, Christer Fuglesang, F. Kajino, A. Murashov, F. Bisconti, Matteo Battisti
Přispěvatelé: AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Organisation de Micro-Électronique Générale Avancée (OMEGA), École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS)
Jazyk: angličtina
Rok vydání: 2020
Předmět:
Meteors
Field of view
7. Clean energy
01 natural sciences
law.invention
High Energy Physics - Experiment
High Energy Physics - Experiment (hep-ex)
law
Earth ionosphere
ultraviolet
optical
[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]
Ultra-high-energy cosmic ray
010303 astronomy & astrophysics
matter: strangeness
Ultraviolet telescopes
Physics
Ultra-high-energy cosmic radiation
photomultiplier
photon
Atmosphere of Earth
infrared
Astrophysics - Instrumentation and Methods for Astrophysics
Space debris
Lightning
Earth atmosphere
lens
air
tube
satellite
FOS: Physical sciences
Cosmic ray
Telescope
0103 physical sciences
International Space Station
surface
14. Life underwater
cosmic radiation: UHE
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Instrumentation and Methods for Astrophysics (astro-ph.IM)
spatial resolution
quark: matter
showers: atmosphere
010308 nuclear & particles physics
Astronomy
resolution
Astronomy and Astrophysics
sensitivity
laser
13. Climate action
Space and Planetary Science
atmosphere
Satellite
Zdroj: The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2021, 253 (2), pp.36. ⟨10.3847/1538-4365/abd93d⟩
Astrophys.J.Suppl.
Astrophys.J.Suppl., 2021, 253 (2), pp.36. ⟨10.3847/1538-4365/abd93d⟩
ISSN: 0004-637X
1538-4357
Popis: Mini-EUSO is a telescope observing the Earth in the ultraviolet band from the International Space Station. It is a part of the JEM-EUSO program, paving the way to future larger missions, such as KEUSO and POEMMA, devoted primarily to the observation of Ultra High Energy Cosmic Rays from space. Mini-EUSO is capable of observing Extensive Air Showers generated by Ultra-High Energy Cosmic Rays with an energy above 10^21 eV and detect artificial showers generated with lasers from the ground. Other main scientific objectives of the mission are the search for nuclearites and Strange Quark Matter, the study of atmospheric phenomena such as Transient Luminous Events, meteors and meteoroids, the observation of sea bioluminescence and of artificial satellites and man-made space debris. Mini-EUSO will map the night-time Earth in the UV range (290 - 430 nm), with a spatial resolution of about 6.3 km and a temporal resolution of 2.5 microseconds, through a nadir-facing UV-transparent window in the Russian Zvezda module. The instrument, launched on August 22, 2019 from the Baikonur cosmodrome, is based on an optical system employing two Fresnel lenses and a focal surface composed of 36 Multi-Anode Photomultiplier tubes, 64 channels each, for a total of 2304 channels with single photon counting sensitivity and an overall field of view of 44 degrees. Mini-EUSO also contains two ancillary cameras to complement measurements in the near infrared and visible ranges. In this paper we describe the detector and present the various phenomena observed in the first months of operations.
23 pages, 20 figures
Databáze: OpenAIRE