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Featured researches published by G. Sáez Cano.


Journal of Physics: Conference Series | 2012

Observation of ultra-high energy cosmic rays in cloudy conditions by the space-based JEM-EUSO Observatory

G. Sáez Cano; J. A. Morales de los Ríos; K Shinozaki; S. Briz; Humberto Prieto; L. del Peral; J. H. Carretero; A. J. de Castro; Francisco Cortes; F. López; A Neromov; Satoshi Wada; M. D. Rodríguez Frías

JEM-EUSO is a space observatory that will be located on-board the Japanese Experiment Module at the International Space Station. It will observe Extensive Air Showers (EAS) induced by ultra-high energy cosmic rays using the Earths atmosphere as detector. In addition to clear sky observations, EAS are also observable in cloudy conditions if a sufficiently large part of the EAS development occurs above the cloud. The atmospheric monitoring system plays a fundamental role in our understanding of the atmospheric conditions in the field of view of the telescope.


Archive | 2015

Observation of Ultra-High Energy Cosmic Rays in cloudy conditions by the JEM-EUSO Space Observatory

G. Sáez Cano; L. del Peral; Francesco Fenu; Rodríguez Frías; A. Santangelo; Johnatan Hernández; Humberto Prieto; J. A. Morales de los Ríos; Kenji Shinozaki; N. Pacheco Gomez

Source of Ultra-high Energy Cosmic Rays (several times 10 19 eV) are still unidentified. Overcoming their extremely small fluxes, a detector with huge observation are as is needed to investigate the energy and arrival direction distribution of EECRs. JEM-EUSO is a unique experiment that will be located in the International Space Station to observe extensive air showers (EAS) by monitoring night part of Earth atmosphere. In addition to clear sky condition, the extensive air showers in cloudy condition are also observable by taking advantage of the certain fraction of EAS develop above the cloud. In the preset work, using Monte Carlo simultions for test clouds, the cloud impact to the trigger efficiency was estimated taking into account the statistics of cloud property.


Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015) | 2016

Cloud Optical Depth obtained from the Infrared Camera data and the UV Flashers mounted on a helicopter flying under the EUSO

G. Sáez Cano; Luis del Peral; malek mastafa; Jorge Fernandez Soriano; James H. Adams; L. Wiencke; Laura López; A. Merino; Marcos Reyes; Enrique Joven; Y. Martín; Elena Roibás; Angel Pedro Sanz; J.L. Sánchez; S. Franchini; J. Licandro; Maria Rodriguez Frias

Spain. 2 ISDC, Astronomy Dept. University of Geneva, Switzerland. 3 University of Alabama in Huntsville (UAH), Huntsville, USA. 4 Colorado School of Mines, Golden, USA. 5 GFA. IMA. University of León, León, Spain. 6 Instituto de Astrofísica de Canarias (IAC), Vía Lactea S/N, Tenerife, Spain. 7 IDR/UPM, E. T. S. I. Aeronáutica y del Espacio, Universidad Politécnica de Madrid, Spain. 8 IFIC, CSIC, U. de València. Dpto. Física Atómica, Molecular y Nuclear, U. de València, Spain.


Advances in Space Research | 2014

Performance and air-shower reconstruction techniques for the JEM-EUSO mission

M. Bertaina; S. Biktemerova; K. Bittermann; Pavol Bobik; D. Campana; F. Fenu; A. Gorgi; F. Guarino; A. Guzmán; K. Higashide; G. Medina-Tanco; Thomas Mernik; D. Naumov; Marián Putiš; M. D. Rodríguez Frías; G. Sáez Cano; A. Santangelo; Kenji Shinozaki; S. Toscano


Archive | 2011

Requirements and Expected Performances of the JEM-EUSO mission

M. Bertaina; A. Santangelo; Kenji Shinozaki; Francesco Fenu; Thomas Mernik; Pavol Bobik; F. Garino; K. Higashide; G. Medina Tanco; G. Sáez Cano; Saitama Univer


EPJ Web of Conferences | 2013

Performances of JEM-EUSO

Mario E. Bertaina; Pavol Bobik; F. Fenu; F. Garino; A. Guzmán; K. Higashide; G. Medina Tanco; Thomas Mernik; G. Sáez Cano; A. Santangelo; Kenji Shinozaki

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Pavol Bobik

Slovak Academy of Sciences

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Francesco Fenu

Istituto Nazionale di Fisica Nucleare

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A. Guzmán

University of Tübingen

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F. Fenu

University of Tübingen

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G. Medina Tanco

National Autonomous University of Mexico

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