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

Bacholle, S.; Barrillon, P.; Battisti, M.; Belov, A.; Bertaina, M.; Bisconti, F.; Blaksley, C.; Blin-Bondil, S.; Cafagna, F.; Cambiè, G.; Capel, F.; Casolino, M.; Crisconio, M.; Churilo, I.; Cotto, G.; de la Taille, C.; Djakonow, A.; Ebisuzaki, T.; Fenu, F.; Franceschi, A.; Fuglesang, C.; Gorodetzky, P.; Haungs, A.; Kajino, F.; Kasuga, H.; Khrenov, B.; Klimov, P.; Kochepasov, S.; Kuznetsov, V.; Marcelli, L.; Marszal, W.; Mignone, M.; Mascetti, G.; Miyamoto, H.; Murashov, A.; Napolitano, T.; Olinto, A. V.; Ohmori, H.; Osteria, G.; Panasyuk, M.; Porfilio, M.; Poroshin, A.; Parizot, E.; Picozza, P.; Piotrowski, L. W.; Plebaniak, Z.; Prevot, G.; Przybylak, M.; Reali, E.; Ricci, M.; Sakaki, N.; Shinozaki, K.; Szabelski, J.; Takizawa, Y.; Turriziani, S.; Valentini, M. Traiche G.; Wada, S.; Wiencke, L.; Yashin, I.; Zuccaro-Marchi, A.

doi:10.48550/arxiv.2010.01937

2020

DOI: 10.48550/arxiv.2010.01937

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

S. Bacholle,

P. Barrillon,

M. Battisti

et al.

Abstract: 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 K-EUSO 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

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“…Mini-EUSO has demonstrated the capability to detect meteors [18]. Indeed Mini-EUSO (at an orbit of 400 km) is sensitive to meteors of apparent magnitude m = 6, whereas POEMMA (at an orbit of 525 km) will be able to detect meteors of m = 10.…”

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confidence: 99%

Prospects for macroscopic dark matter detection at space-based and suborbital experiments

Anchordoqui¹,

Bertaina²,

Casolino³

et al. 2021

EPL

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We compare two different formalisms for modeling the energy deposition of macroscopically sized/massive quark nuggets (also known as macros) in the Earth's atmosphere. We show that for a reference mass of 1 g, there is a discrepancy in the macro luminosity of about 14 orders of magnitude between the predictions of the two formalisms. Armed with our finding we estimate the sensitivity for macro detection at space-based (Mini-EUSO and POEMMA) and suborbital (EUSO-SPB2) experiments.

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mentioning

confidence: 99%

Prospects for macroscopic dark matter detection at space-based and suborbital experiments

Anchordoqui¹,

Bertaina²,

Casolino³

et al. 2021

EPL

View full text Add to dashboard Cite

show abstract

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

Cited by 1 publication

References 34 publications

Prospects for macroscopic dark matter detection at space-based and suborbital experiments

Prospects for macroscopic dark matter detection at space-based and suborbital experiments

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