Ultra high energy cosmic ray detector KLYPVE on board the Russian Segment of the ISS

Panasyuk, M. I.; Климов, П. А.; Khrenov, B. A.; Sharakin, S.; Zotov, Mikhail; Picozza, P.; Casolino, M.; Ebisuzaki, Toshikazu; Gorodetzky, P.

doi:10.22323/1.236.0669

Cited by 18 publications

(16 citation statements)

References 16 publications

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“…In the JEM-EUSO Collaboration, a large Fresnel lens telescope was developed (Adams et al, 2015). In Russia, detectors that use concentrator mirrors for collecting fluorescence light, TUS (Klimov et al, 2017) and KLYPVE (Panasyuk et al, 2016), were proposed and developed.…”

Section: The Current Status and Perspectives Of Space Experiments To mentioning

confidence: 99%

“…Another, much larger space instrument, KLYPVE, is being developed in close cooperation with the JEM-EUSO Collaboration and is known as KLYPVE-EUSO (K-EUSO) (Panasyuk et al, 2016). To fulfill the requirements of the K-EUSO experiment, a Schmidt UV telescope covering a FOV of 40 • with an entrance pupil diameter of 2.5 m, and a 4 m diameter mirror was developed.…”

Section: The Current Status and Perspectives Of Space Experiments To mentioning

confidence: 99%

See 1 more Smart Citation

Open Questions in Cosmic-Ray Research at Ultrahigh Energies

Batista

Biteau

Bustamante

et al. 2019

Front. Astron. Space Sci.

211

119

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We review open questions and prospects for progress in ultrahigh-energy cosmic ray (UHECR) research, based on a series of discussions that took place during the "The High-Energy Universe: Gamma-Ray, Neutrino, and Cosmic-ray Astronomy" MIAPP workshop in 2018. Specifically, we overview open questions on the origin of the bulk of UHECRs, the UHECR mass composition, the origin of the end of the cosmic-ray spectrum, the transition from Galactic to extragalactic cosmic rays, the effect of magnetic fields on the trajectories of UHECRs, anisotropy expectations for specific astrophysical scenarios, hadronic interactions, and prospects for discovering neutral particles as well as new physics at ultrahigh energies. We also briefly overview upcoming and proposed UHECR experiments and discuss their projected science reach.

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Section: The Current Status and Perspectives Of Space Experiments To mentioning

confidence: 99%

Section: The Current Status and Perspectives Of Space Experiments To mentioning

confidence: 99%

Open Questions in Cosmic-Ray Research at Ultrahigh Energies

Batista

Biteau

Bustamante

et al. 2019

Front. Astron. Space Sci.

211

119

View full text Add to dashboard Cite

show abstract

“…To eliminate the off-axis aberration an additional corrective element was introduced into the telescope system in form of a Fresnel lens in front of the photodetector. Two versions of the detector were developed: Baseline and Mylti-Eye Telescope System (METS) [9,10]. 1 1 EeV = 10 18 eV 2 KLYPVE is a Russian acronym for extreme energy cosmic rays.…”

Section: From Klypve To K-eusomentioning

confidence: 99%

Status of the KLYPVE-EUSO detector for EECR study on board the ISS

Климов¹,

Casolino²

2017

Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017)

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For the JEM-EUSO CollaborationKLYPVE-EUSO is a mission led by the Russian Space Agency to place an ultra-high energy cosmic ray observatory on board the Russian Segment (RS) of the ISS. The concept of the detector is based on the mirror-type detector proposed by SINP MSU in 2010 and improved by the joint studies with the JEM-EUSO collaboration. The current configuration is based on a Schmidt type optical system. This allows to increase the Field of View to 40 degrees and makes the experiment competitive with large ground-based observatories, with the advantage of the uniform exposure over the whole celestial sphere. The laboratory models of mirror-concentrator and photo detector module are being developed and manufactured. The launch of the experiment is scheduled to 2022 followed by the installation on the RS of the ISS and at least two years of operation.

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“…The threshold will be lower than that of JEM-EUSO thanks to the larger collection efficiency of the reflective optics. Details can be found in [25], [26], [27]. The mission is planned to be launched in 2020.…”

Section: Pos(icrc2015)618mentioning

confidence: 99%