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Wyszukujesz frazę "Kuznetsov, G. V." wg kryterium: Wszystkie pola


Tytuł:
Improvement of the regenerating energy accounting system on the direct current railways
Autorzy:
Kuznetsov, V. G.
Sablin, O. I.
Chornaya, A. V.
Tematy:
energy accounting system
power consumption
power supply
traffic size
regeneration
system rozliczeniowy energii
pobór mocy
zasilanie
wielkość ruchu
regeneracja
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Czytelnia Czasopism PAN
Powiązania:
https://bibliotekanauki.pl/articles/224043.pdf  Link otwiera się w nowym oknie
Opis:
Purpose. Monitoring of current state of quantitative indices of regenerative energy in the suburban movement, the analysis of the factors influencing its volumes and improvement the principles of the train regenerative energy accounting on the basis of it. Relevance. Development of effective measures of increase the regeneration efficiency of the electric power in system of electric traction demands comprehensive completeness of information on quantitative indices of regeneration energy volumes at all possible levels of its analysis, in particular on the corresponding sections of RS movement that will allow to establish the influence on the level of regeneration of various factors, such as parameters of traction power supply and the organization of train service. As the existing system of the regenerative energy accounting does not allow to consider the specified factors, development of the principles for increasing the efficiency of the analysis of volumes of return energy to a contact line during regenerative braking on DC rolling stock is the actual direction of researches. Collective monitoring of regeneration energy volumes by specialists of locomotive service, power supply and traffic operating departments will be essentially new approach to definition of real factors and taking effective decisions for increasing of using of regenerative energy. Scientific novelty. It’s offered to consider the influence on quantitative indices of regenerative energy the parameters of traction power supply and the organization (sizes) of traffic service on sections. Practical importance. Increasing the efficiency of the regeneration energy accounting is an important element in drawing up the balance of energy for electric traction system, development of the effective methods for improvement of the conditions of regeneration in it and in estimation of its power indicators in general.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
δ13 C variation in carbonate platform sediments of the Northern Tethys in Late Jurassic
Autorzy:
Rudko, S.V.
Kuznetsov, A.B.
Pokrovsky, B.G.
Tematy:
paleogeographical model
paleoecological model
inclination
Pokaż więcej
Wydawca:
Akademia Górniczo-Hutnicza im. Stanisława Staszica w Krakowie. Wydawnictwo AGH
Powiązania:
https://bibliotekanauki.pl/articles/184621.pdf  Link otwiera się w nowym oknie
Opis:
Сarbon isotopic composition of Late Jurassic sediments displays a trend of 13 C depletion in the World ocean. Meanwhile, depending on local paleogeographical conditions, δ 13 C curves for different palaeoprovinces differ in inclinations and absolute values (Nunn & Price 2010). That is why a separate δ 13 C curve needs to be developed for every specific region. After such development, the inverse problem – correlation of the sedimentary complex by comparing δ 13 C parameters – can be solved. A comparison of δ 13 C values in contemporaneous sediments can be also used as an instrument for testing paleogeographical and paleoecological models. Previous δ 13 C data for the Upper Jurassic sediments of the Tethys region were obtained for its Western passive margin and Central Atlantics (Padden et al. 2002, Coimbra et al. 2009). These data have been acquired from precisely dated hemipelagic sediments containing index fauna and epioceanic Ammonitico-Rosso facies. In the current study we present δ 13 C variations in carbonate platform sediments from the backarc basin of the Northern Tethys (N20° to N40°) (Meijers et al. 2010) mostly based on Sr-chemostratigraphic correlation and dating of carbonate complexes. We studied Sr, C and O isotopic composition of the Upper Jurassic carbonate complexes of the Crimean Mountains. These complexes were formed under different conditions: Kimmeridgian and Early Tithonian sediments were deposited in shallow-water carbonate platform settings. In most cases they lack index fossils and their age is defined by Sr-chemostratigraphy (Rudko et al. 2014); Late Tithonian to Early Berriasian sediments were sampled from a carbonate platform reef facies, slope and toe of slope carbonate megabreccias. Reef and breccias deposits were dated using Sr-chemostratigraphy, and confirmed by calpionellide biostratigraphy. In the absence of well preserved faunal remnants in the studied sections, limestone samples with the best preservation of primary sedimentary textures were collected for Sr isotopic–geochemical studies. Samples with large calcite veins or abundant epigenetic sparite were excluded from this research. Limestone samples for reconstructing the 87 Sr/ 86 Sr isotopic parameters of depositional environments were selected using geochemical criteria (Mn/Sr < 0.2, Fe/Sr < 1.6, Mg/Ca < 0.024; δ 18 О > −1.5‰) and subjected to preliminary treatment in a 1 N ammonium acetate solution. From more then 100 analyzed samples only 13 best preserved were used to provide correlation between sections and the age of strata. Most of samples used to determine C isotopic composition are represented by micritic limestones with low content of sparry cements and fragments of primary aragonitic grains. The content of insoluble impurities in limestones does not exceed 9%. All selected samples display no correlation between the amount of siliciclastic impurities, δ 13 C and δ 18 О values. δ 13 C values in the measured samples vary between +1 and 3.5‰, δ 18 О: from −2.9‰ to +1,3‰. C – isotopic composition in 44 samples was considered to be diagenetically unaffected and they were selected to provide δ 13 C curve. According to the results of comparison of stable isotope composition with microfacies of samples, δ 13 C values are not environment-dependent in contrast to δ 18 О, which are slightly enriched in 18 O in offshore and slope facies. The measured values of δ 13 С are falling from an average 3.2‰ in Late Kimmeridgian through 2.6‰ in Early Tithonian to 1.7‰ in Late Tithonian – Early Berriasian. This corresponds to the global δ 13 С trend in Upper Jurassic sediments (Nunn & Price 2010). Among other Kimmeridgian – Berriasian carbonates the Northern Tethys carbonate platform deposits are 0.5–1‰ higher than δ 13 С from the Western Tethys (Coimbra et al. 2009). The following factors (or their combinations) may explain observed 13 C-enriched isotopic composition of the Northern Tethyan backarc basin deposits: 1. increased amount of shallow-water allochems and cements in the sediments of carbonate platform and its aprons, compared to hemipelagites of Western Tethyan margin; 2. increased bioproductivity of photosynthetic organisms – cyanobacteria and green algae that played an important role in the studied Upper Jurassic carbonate platform deposits (Krajewski 2010, Piskunov et al. 2012, Bucur et al. 2014), removed large quantity of light carbon from water, leading to 13 C enrichment of bicarbonate. It is interesting to note that volcanic activity on Tethyan active margin seems not to have an impact on δ 13 С values of the studied sediments.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
The Revised Method for Calculating of The Optimal Train Control Mode
Autorzy:
Zhelieznov, Konstantun I.
Akulov, Artem S.
Zabolotniy, Oleksandr M.
Ursulyak, Lyudmila V.
Chabanuk, Evgenij V.
Shvets, Angela O.
Kuznetsov, Valeriy G.
Radkevych, Anatolii V.
Tematy:
conducting a train
running profile of the train
optimal control
driving simulators
electric traction motors
prowadzenia pociągu
profil jazdy pociągu
optymalna kontrola
symulator jazdy
silnik trakcyjny
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Czytelnia Czasopism PAN
Powiązania:
https://bibliotekanauki.pl/articles/224041.pdf  Link otwiera się w nowym oknie
Opis:
Development of a method for calculating the optimal mode of conducting a train in terms of energy saving meet the safety requirements and schedules. The method of calculation must solve the assigned tasks without significant time spent on the calculation. To implement this method of calculation was used a simplified model of the train as a controlled system. The existing mathematical and algorithmic methods for solving isoperimetric problems of finding the optimal solution in the presence of restrictions on resources were the information base for methodology development. Scientific works of domestic and foreign scientists, professional periodicals, materials of scientific and practical conferences, methodical and normative materials, currently in force on Ukrainian Railways. The results of these studies were used to create simulators on the basis of computer technology for the training of locomotive drivers. The scientific novelty of the proposed calculation method consists in applying the simplified calculations of the status of the train as a controlled system, without the use of differential equations of motion that allows to significantly increase the speed of the calculations. This, in turn, will solve the problems of finding optimal control in real time, taking into account changing conditions during the movement of the train. The practical significance of the obtained results is the use of such a calculation method that does not require significant time for its implementation and can be used as a subsystem of the on-board train control system capable of performing calculations taking into account changes in the current train situation.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Ultra high energy photons and neutrinos with JEM-EUSO
Autorzy:
Cremonini, R.
Belov, K.
Blin-Bondil, S.
Crawford, H. J.
Gonchar, M.
Tsenov, R.
Hernández Carretero, J.
Vigorito, C.
Asano, K.
Włodarczyk, Z.
Villaseñor, L.
Bonamente, M.
Rothkaehl, H.
Kaneko, I.
Flamini, M.
Wibig, T.
Sharakin, S.
Sato, M.
Yoshida, S.
Finco, D.
Shirahama, T.
Osteria, G.
Sato, H.
Neronov, A.
Lacombe, M.
Rusinov, I.
Connaughton, V.
Briggs, M. S.
Vaduvescu, O.
Distratis, G.
Szabelska, B.
Yamamoto, Y.
Tokuno, H.
Lee, J.
Olinto, A. V.
Insolia, A.
Caruso, R.
Bertaina, M.
López, F.
Roudil, G.
Harlov, B.
Higashide, K.
Weber, M.
Judd, E. G.
Piraino, S.
Pastircak, B.
Pollini, A.
Nagataki, S.
Sarazin, F.
Kim, J.-S.
Yonetoku, D.
Scotti, V.
Unger, M.
Andreev, V.
Valore, L.
Adams Jr, J. H.
Takahashi, Y.
Kudela, K.
Young, R.
Jung, A.
Csorna, S.
Nava, R.
Watts, J., Jr
Supanitsky, D.
Giraudo, G.
Panasyuk, M. I.
Ikeda, H.
Miyamoto, H.
Bayer, J.
Di Martino, M.
Masciantonio, G.
Lim, H.
Anchordoqui, L.
Modestino, G.
Segreto, A.
Ogio, S.
Karus, M.
Barrillon, P.
Morozenko, V. S.
Takami, H.
Park, I. H.
Picozza, P.
Fenu, F.
Engel, R.
Słomińska, K.
Tkachev, L.
Schanz, T.
Joven, E.
Gorodetzky, P.
Cellino, A.
Galeotti, P.
Perez Cano, S.
Reardon, P.
Tajima, F.
Ahmad, S.
Blaksley, C.
Dulucq, F.
Sakaki, N.
Casolino, M.
Fornaro, C.
Nakamura, T.
Wada, S.
Karczmarczyk, J.
Sobey, A.
Conti, L.
Bruno, A.
Klimov, P. A.
Peter, T.
Nagano Murakami, M.
Kajino, T.
Licandro, J.
Prat, P.
Roth, M.
De Santis, C.
Kusenko, A.
Kawasaki, Y.
Dagoret-Campagne, S.
Vankova, G.
Matev, R.
Allard, D.
Tenzer, C.
Belenguer, T.
Sakata, M.
Santangelo, A.
Ogawa, T.
Sugiyama, T.
Albert, J.-N.
Biermann, P. L.
Fernández-Gómez, I.
Guzmán, A.
Nagata, M.
Paul, T.
Salazar, H.
Wilms, J.
Silva López, H. H.
Lachaud, C.
Rodríguez Frías, M. D.
Shimizu, H. M.
Nonaka, T.
Franceschi, A.
Kawai, K.
Trillaud, F.
Mase, K.
Mot, B.
Kajino, F.
Campana, D.
Cline, D.
Orleański, P.
Ronga, F.
Rybczyński, M.
Sabau, M. D.
Ebisuzaki, T.
Bechini, R.
Mernik, T.
Tajima, T.
Baragatti, P.
Tsunesada, Y.
Christl, M. J.
Yamamoto, T.
de Castro, A. J.
Sánchez, S.
Yashin, I. V.
Sledd, J.
Hachisu, Y.
Prévôt, G.
Serra, M.
Dell’Oro, A.
González Alvarado, C.
Kurihara, Y.
Wille, M.
De Donato, C.
Ikeda, D.
Vallania, P.
Shibata, T.
Biktemerova, S.
Maccarone, M. C.
Szabelski, J.
Yoshida, K.
Santiago Crúz, L.
Bellotti, R.
Inoue, S.
Bogomilov, M.
Murakami, T.
Rodríguez, I.
Monnier-Ragaigne, D.
Fang, K.
Tsuno, K.
Arai, Y.
Kleifges, M.
Uchihori, Y.
Chikawa, M.
Suzuki, M.
Bobik, P.
Garipov, G.
Briz, S.
Tymieniecka, T.
von Ballmoos, P.
Karadzhov, Y.
Putis, M.
Kuznetsov, E.
Marcelli, L.
Toscano, S.
Mizumoto, Y.
Geary, J.
Gelmini, G.
Ferrarese, S.
Kim, S.-W.
Isgrò, F.
Saito, A.
Selmane, S.
De Simone, N.
Maravilla, D.
Monaco, A.
Blümer, J.
Miyazaki, Y.
Ebersoldt, A.
Takizawa, Y.
Blanc, N.
Ohmori, H.
Cafagna, F.
Marini, A.
Tajima, N.
Schieler, H.
Berlind, A. A.
Guarino, F.
Katahira, K.
Napolitano, T.
Kolev, D.
Ave Pernas, M.
Patzak, T.
Weiler, T. J.
Wiencke, L.
Zotov, M. Yu.
Błęcki, J.
Tomida, T.
Semikoz, D.
Mannheim, K.
Plebaniak, Z.
Keilhauer, B.
del Peral, L.
Martinez, O.
Nomoto, K.
Inoue, N.
Takeda, M.
Medina-Tanco, G.
Catalano, C.
Zuccaro Marchi, A.
de la Taille, C.
Yang, J.
Watanabe, S.
Castellinic, G.
Naumov, D.
Piotrowski, L. W.
Morales de los Ríos, J. A.
Sáez-Cano, G.
Falk, S.
Moretto, C.
Haungs, A.
Siemieniec-Oziębło, Grażyna
Shinozaki, K.
Valdés-Galicia, J. F.
Parizot, E.
Catalano, G.
Batsch, T.
Itow, Y.
Park, H. W.
Tone, N.
Yano, H.
Reyes, M.
Pennypacker, C.
Watanabe, J.
Dupieux, M.
Prieto, H.
Saprykin, O.
Kreykenbohm, I.
Cordero, G.
Cassardo, C.
Ricci, M.
Anzalone, A.
Pierog, T.
Fujimoto, J.
Sanz Palomino, M.
Sagawa, H.
Tibolla, O.
Khrenov, B. A.
Capdevielle, J.-N.
Fukushima, M.
Opis:
Ultra high energy photons and neutrinos are carriers of very important astrophysical information. They may be produced at the sites of cosmic ray acceleration or during the propagation of the cosmic rays in the intergalactic medium. In contrast to charged cosmic rays, photon and neutrino arrival directions point to the production site because they are not deflected by the magnetic fields of the Galaxy or the intergalactic medium. In this work we study the characteristics of the longitudinal development of showers initiated by photons and neutrinos at the highest energies. These studies are relevant for development of techniques for neutrino and photon identification by the JEM-EUSO telescope. In particular, we study the possibility of observing the multi-peak structure of very deep horizontal neutrino showers with JEM-EUSO. We also discuss the possibility to determine the flavor content of the incident neutrino flux by taking advantage of the different characteristics of the longitudinal profiles generated by different type of neutrinos. This is of grate importance for the study of the fundamental properties of neutrinos at the highest energies. Regarding photons, we discuss the detectability of the cosmogenic component by JEM-EUSO and also estimate the expected upper limits on the photon fraction which can be obtained from the future JEM-EUSO data for the case in which there are no photons in the samples.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Performances of JEM-EUSO : angular reconstruction
Autorzy:
Panasyuk, M. I.
Mot, B.
Garipov, G.
Nagano Murakami, M.
Keilhauer, B.
Sagawa, H.
Ebersoldt, A.
Kuznetsov, E.
Vankova, G.
Wilms, J.
Picozza, P.
Cordero, G.
Włodarczyk, Z.
Salazar, H.
Briggs, M. S.
Pierog, T.
Fujimoto, J.
Park, H. W.
Neronov, A.
Schanz, T.
Ogawa, T.
Geary, J.
Christl, M. J.
Segreto, A.
Dagoret-Campagne, S.
Bobik, P.
Bertaina, M.
Higashide, K.
Paul, T.
Harlov, B.
Park, I. H.
Vaduvescu, O.
Scotti, V.
Ave Pernas, M.
Kudela, K.
Maccarone, M. C.
Bellotti, R.
Roudil, G.
Catalano, G.
Dulucq, F.
Castellinic, G.
Serra, M.
Franceschi, A.
Itow, Y.
Peter, T.
Gonchar, M.
Masciantonio, G.
Gelmini, G.
Belenguer, T.
Judd, E. G.
Siemieniec-Oziębło, Grażyna
Tone, N.
Kawai, K.
Valdés-Galicia, J. F.
Yamamoto, Y.
Bechini, R.
Sarazin, F.
Yano, H.
Isgrò, F.
Biermann, P. L.
Reyes, M.
Tsenov, R.
Piotrowski, L. W.
Haungs, A.
Mizumoto, Y.
Weber, M.
Miyamoto, H.
Szabelski, J.
Kreykenbohm, I.
Asano, K.
Morales de los Ríos, J. A.
Fernández-Gómez, I.
Conti, L.
Biktemerova, S.
Tomida, T.
Lacombe, M.
Licandro, J.
Karus, M.
Shinozaki, K.
Tibolla, O.
Cline, D.
Bonamente, M.
Miyazaki, Y.
Ahmad, S.
Sáez-Cano, G.
Valore, L.
Sato, H.
Saprykin, O.
Nonaka, T.
Toscano, S.
Sledd, J.
Adams Jr, J. H.
Fukushima, M.
Sakaki, N.
Moretto, C.
Tajima, N.
Takahashi, Y.
Monaco, A.
Marcelli, L.
Briz, S.
Watanabe, J.
Pollini, A.
Vallania, P.
Caruso, R.
Barrillon, P.
Klimov, P. A.
Tajima, F.
Sugiyama, T.
Albert, J.-N.
De Donato, C.
Watanabe, S.
de la Taille, C.
Nagataki, S.
Santangelo, A.
Olinto, A. V.
Sanz Palomino, M.
Sobey, A.
Bogomilov, M.
Mannheim, K.
Wiencke, L.
Inoue, S.
Reardon, P.
Joven, E.
Nakamura, T.
Distratis, G.
Medina-Tanco, G.
Rothkaehl, H.
Sakata, M.
Villaseñor, L.
Young, R.
Bruno, A.
Tenzer, C.
Patzak, T.
González Alvarado, C.
Takizawa, Y.
Kajino, F.
Engel, R.
Inoue, N.
Orleański, P.
Cafagna, F.
Yoshida, K.
Yonetoku, D.
Flamini, M.
Plebaniak, Z.
Saito, A.
Blanc, N.
Galeotti, P.
Rodríguez Frías, M. D.
Santiago Crúz, L.
Putis, M.
Schieler, H.
Hachisu, Y.
Nomoto, K.
Ricci, M.
Arai, Y.
Silva López, H. H.
Berlind, A. A.
Weiler, T. J.
Supanitsky, D.
Mernik, T.
Dupieux, M.
Fornaro, C.
Casolino, M.
Selmane, S.
Andreev, V.
del Peral, L.
Finco, D.
Shibata, T.
Kim, S.-W.
Tymieniecka, T.
Pennypacker, C.
Rusinov, I.
Lachaud, C.
Ferrarese, S.
Ikeda, D.
Karczmarczyk, J.
Chikawa, M.
Takami, H.
Marini, A.
Shirahama, T.
Belov, K.
Guzmán, A.
Tsunesada, Y.
Piraino, S.
Campana, D.
Prat, P.
Rodríguez, I.
Kaneko, I.
Dell’Oro, A.
Ebisuzaki, T.
Kim, J.-S.
Batsch, T.
Nava, R.
Rybczyński, M.
Szabelska, B.
von Ballmoos, P.
Baragatti, P.
Falk, S.
Ogio, S.
Murakami, T.
Capdevielle, J.-N.
Karadzhov, Y.
Sato, M.
Pastircak, B.
Vigorito, C.
Prieto, H.
Prévôt, G.
Tkachev, L.
Blümer, J.
Hernández Carretero, J.
Parizot, E.
López, F.
Allard, D.
Kleifges, M.
Takeda, M.
Tajima, T.
Modestino, G.
Yang, J.
Wada, S.
Katahira, K.
Sharakin, S.
Zuccaro Marchi, A.
Yashin, I. V.
Cellino, A.
Insolia, A.
Ohmori, H.
Maravilla, D.
Nagata, M.
Ikeda, H.
De Santis, C.
Blin-Bondil, S.
Csorna, S.
Napolitano, T.
Osteria, G.
Ronga, F.
Słomińska, K.
Kolev, D.
Di Martino, M.
Morozenko, V. S.
Błęcki, J.
Fang, K.
Jung, A.
Matev, R.
Roth, M.
Anzalone, A.
Kusenko, A.
Trillaud, F.
Wibig, T.
Yamamoto, T.
Blaksley, C.
Guarino, F.
Semikoz, D.
Connaughton, V.
Kawasaki, Y.
Zotov, M. Yu.
De Simone, N.
Catalano, C.
Mase, K.
Anchordoqui, L.
Kajino, T.
Uchihori, Y.
Unger, M.
Sánchez, S.
Suzuki, M.
Cremonini, R.
Fenu, F.
Lim, H.
Lee, J.
Kurihara, Y.
Perez Cano, S.
Giraudo, G.
Shimizu, H. M.
Yoshida, S.
Naumov, D.
Khrenov, B. A.
Monnier-Ragaigne, D.
Tokuno, H.
Cassardo, C.
Bayer, J.
Martinez, O.
Watts, J., Jr
Gorodetzky, P.
Crawford, H. J.
Wille, M.
Tsuno, K.
Sabau, M. D.
de Castro, A. J.
Opis:
Mounted on the International Space Station(ISS), the Extreme Universe Space Observatory, on-board the Japanese Experimental Module (JEM-EUSO), relies on the well established fluorescence technique to observe Extensive Air Showers (EAS) developing in the earth’s atmosphere. Focusing on the detection of Ultra High Energy Cosmic Rays (UHECR) in the decade of 10^{20} eV, JEM-EUSO will face new challenges by applying this technique from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed in this context to provide a full end-to-end simulation frame, and assess the overall performance of the detector. Within ESAF, angular reconstruction can be separated into two conceptually different steps. The first step is pattern recognition, or filtering, of the signal to separate it from the background. The second step is to perform different types of fitting in order to search for the relevant geometrical parameters that best describe the previously selected signal. In this paper, we discuss some of the techniques we have implemented in ESAF to perform the geometrical reconstruction of EAS seen by JEM-EUSO. We also conduct thorough tests to assess the performances of these techniques in conditions which are relevant to the scope of the JEM-EUSO mission. We conclude by showing the expected angular resolution in the energy range that JEM-EUSO is expected to observe.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Performances of JEM–EUSO : energy and X_{max} reconstruction
Autorzy:
Panasyuk, M. I.
Mot, B.
Garipov, G.
Keilhauer, B.
Sagawa, H.
Ebersoldt, A.
Kuznetsov, E.
Vankova, G.
Wilms, J.
Picozza, P.
Cordero, G.
Włodarczyk, Z.
Salazar, H.
Briggs, M. S.
Pierog, T.
Fujimoto, J.
Park, H. W.
Neronov, A.
Schanz, T.
Ogawa, T.
Geary, J.
Christl, M. J.
Segreto, A.
Dagoret-Campagne, S.
Bobik, P.
Bertaina, M.
Higashide, K.
Paul, T.
Harlov, B.
Park, I. H.
Vaduvescu, O.
Scotti, V.
Ave Pernas, M.
Kudela, K.
Maccarone, M. C.
Murakami, M. Nagano
Bellotti, R.
Roudil, G.
Catalano, G.
Dulucq, F.
Castellinic, G.
Serra, M.
Franceschi, A.
Itow, Y.
Peter, T.
Gonchar, M.
Masciantonio, G.
Gelmini, G.
Belenguer, T.
Judd, E. G.
Siemieniec-Oziębło, Grażyna
Tone, N.
Kawai, K.
Valdés-Galicia, J. F.
Yamamoto, Y.
Bechini, R.
Sarazin, F.
Yano, H.
Isgrò, F.
Biermann, P. L.
Reyes, M.
Tsenov, R.
Piotrowski, L. W.
Haungs, A.
Mizumoto, Y.
Weber, M.
Miyamoto, H.
Szabelski, J.
Kreykenbohm, I.
Asano, K.
Morales de los Ríos, J. A.
Fernández-Gómez, I.
Conti, L.
Biktemerova, S.
Tomida, T.
Lacombe, M.
Licandro, J.
Karus, M.
Shinozaki, K.
Tibolla, O.
Cline, D.
Bonamente, M.
Miyazaki, Y.
Ahmad, S.
Sáez-Cano, G.
Valore, L.
Sato, H.
Saprykin, O.
Nonaka, T.
Toscano, S.
Sledd, J.
Adams Jr, J. H.
Fukushima, M.
Sakaki, N.
Moretto, C.
Tajima, N.
Takahashi, Y.
Monaco, A.
Marcelli, L.
Briz, S.
Watanabe, J.
Pollini, A.
Vallania, P.
Caruso, R.
Barrillon, P.
Klimov, P. A.
Tajima, F.
Sugiyama, T.
Albert, J.-N.
De Donato, C.
Watanabe, S.
de la Taille, C.
Nagataki, S.
Santangelo, A.
Olinto, A. V.
Sanz Palomino, M.
Sobey, A.
Bogomilov, M.
Mannheim, K.
Wiencke, L.
Inoue, S.
Reardon, P.
Joven, E.
Nakamura, T.
Distratis, G.
Medina-Tanco, G.
Rothkaehl, H.
Sakata, M.
Villaseñor, L.
Young, R.
Bruno, A.
Tenzer, C.
Patzak, T.
González Alvarado, C.
Takizawa, Y.
Kajino, F.
Engel, R.
Inoue, N.
Orleański, P.
Cafagna, F.
Yoshida, K.
Yonetoku, D.
Flamini, M.
Plebaniak, Z.
Saito, A.
Blanc, N.
Galeotti, P.
Rodríguez Frías, M. D.
Santiago Crúz, L.
Putis, M.
Schieler, H.
Hachisu, Y.
Nomoto, K.
Ricci, M.
Arai, Y.
Silva López, H. H.
Berlind, A. A.
Weiler, T. J.
Supanitsky, D.
Mernik, T.
Dupieux, M.
Fornaro, C.
Casolino, M.
Selmane, S.
Andreev, V.
del Peral, L.
Finco, D.
Shibata, T.
Kim, S.-W.
Tymieniecka, T.
Pennypacker, C.
Rusinov, I.
Lachaud, C.
Ferrarese, S.
Ikeda, D.
Karczmarczyk, J.
Chikawa, M.
Takami, H.
Marini, A.
Shirahama, T.
Belov, K.
Guzmán, A.
Tsunesada, Y.
Piraino, S.
Campana, D.
Prat, P.
Rodríguez, I.
Kaneko, I.
Dell’Oro, A.
Ebisuzaki, T.
Kim, J.-S.
Batsch, T.
Nava, R.
Rybczyński, M.
Szabelska, B.
von Ballmoos, P.
Baragatti, P.
Falk, S.
Ogio, S.
Murakami, T.
Capdevielle, J.-N.
Karadzhov, Y.
Sato, M.
Pastircak, B.
Vigorito, C.
Prieto, H.
Prévôt, G.
Tkachev, L.
Blümer, J.
Hernández Carretero, J.
Parizot, E.
López, F.
Allard, D.
Kleifges, M.
Takeda, M.
Tajima, T.
Modestino, G.
Yang, J.
Wada, S.
Katahira, K.
Sharakin, S.
Zuccaro Marchi, A.
Yashin, I. V.
Cellino, A.
Insolia, A.
Ohmori, H.
Maravilla, D.
Nagata, M.
Ikeda, H.
De Santis, C.
Blin-Bondil, S.
Csorna, S.
Napolitano, T.
Osteria, G.
Ronga, F.
Słomińska, K.
Kolev, D.
Di Martino, M.
Morozenko, V. S.
Błęcki, J.
Fang, K.
Jung, A.
Matev, R.
Roth, M.
Anzalone, A.
Kusenko, A.
Trillaud, F.
Wibig, T.
Yamamoto, T.
Blaksley, C.
Guarino, F.
Semikoz, D.
Connaughton, V.
Kawasaki, Y.
Zotov, M. Yu.
De Simone, N.
Catalano, C.
Mase, K.
Anchordoqui, L.
Kajino, T.
Uchihori, Y.
Unger, M.
Sánchez, S.
Suzuki, M.
Cremonini, R.
Fenu, F.
Lim, H.
Lee, J.
Kurihara, Y.
Perez Cano, S.
Giraudo, G.
Shimizu, H. M.
Yoshida, S.
Naumov, D.
Khrenov, B. A.
Monnier-Ragaigne, D.
Tokuno, H.
Cassardo, C.
Bayer, J.
Martinez, O.
Watts, J., Jr
Gorodetzky, P.
Crawford, H. J.
Wille, M.
Tsuno, K.
Sabau, M. D.
de Castro, A. J.
Opis:
The Extreme Universe Space Observatory (EUSO) on–board the Japanese Experimental Module (JEM) of the International Space Station aims at the detection of ultra high energy cosmic rays from space. The mission consists of a UV telescope which will detect the fluorescence light emitted by cosmic ray showers in the atmosphere. The mission, currently developed by a large international collaboration, is designed to be launched within this decade. In this article, we present the reconstruction of the energy of the observed events and we also address the X_{max} reconstruction. After discussing the algorithms developed for the energy and X_{max} reconstruction, we present several estimates of the energy resolution, as a function of the incident angle, and energy of the event. Similarly, estimates of the X_{max} resolution for various conditions are presented.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
The JEM-EUSO instrument
Autorzy:
Panasyuk, M. I.
Mot, B.
Garipov, G.
Nagano Murakami, M.
Keilhauer, B.
Sagawa, H.
Ebersoldt, A.
Kuznetsov, E.
Vankova, G.
Wilms, J.
Picozza, P.
Cordero, G.
Włodarczyk, Z.
Salazar, H.
Briggs, M. S.
Pierog, T.
Fujimoto, J.
Park, H. W.
Neronov, A.
Schanz, T.
Ogawa, T.
Geary, J.
Christl, M. J.
Segreto, A.
Dagoret-Campagne, S.
Bobik, P.
Bertaina, M.
Higashide, K.
Paul, T.
Harlov, B.
Park, I. H.
Vaduvescu, O.
Scotti, V.
Ave Pernas, M.
Kudela, K.
Maccarone, M. C.
Bellotti, R.
Roudil, G.
Catalano, G.
Dulucq, F.
Castellinic, G.
Serra, M.
Franceschi, A.
Itow, Y.
Peter, T.
Gonchar, M.
Masciantonio, G.
Gelmini, G.
Belenguer, T.
Judd, E. G.
Siemieniec-Oziębło, Grażyna
Tone, N.
Kawai, K.
Valdés-Galicia, J. F.
Yamamoto, Y.
Bechini, R.
Sarazin, F.
Yano, H.
Isgrò, F.
Biermann, P. L.
Reyes, M.
Tsenov, R.
Piotrowski, L. W.
Haungs, A.
Mizumoto, Y.
Weber, M.
Miyamoto, H.
Szabelski, J.
Kreykenbohm, I.
Asano, K.
Morales de los Ríos, J. A.
Fernández-Gómez, I.
Conti, L.
Biktemerova, S.
Tomida, T.
Lacombe, M.
Licandro, J.
Karus, M.
Shinozaki, K.
Tibolla, O.
Cline, D.
Bonamente, M.
Miyazaki, Y.
Ahmad, S.
Sáez-Cano, G.
Valore, L.
Sato, H.
Saprykin, O.
Nonaka, T.
Toscano, S.
Sledd, J.
Adams Jr, J. H.
Fukushima, M.
Sakaki, N.
Moretto, C.
Tajima, N.
Takahashi, Y.
Monaco, A.
Marcelli, L.
Briz, S.
Watanabe, J.
Pollini, A.
Vallania, P.
Caruso, R.
Barrillon, P.
Klimov, P. A.
Tajima, F.
Sugiyama, T.
Albert, J.-N.
De Donato, C.
Watanabe, S.
de la Taille, C.
Nagataki, S.
Santangelo, A.
Olinto, A. V.
Sanz Palomino, M.
Sobey, A.
Bogomilov, M.
Mannheim, K.
Wiencke, L.
Inoue, S.
Reardon, P.
Joven, E.
Nakamura, T.
Distratis, G.
Medina-Tanco, G.
Rothkaehl, H.
Sakata, M.
Villaseñor, L.
Young, R.
Bruno, A.
Tenzer, C.
Patzak, T.
González Alvarado, C.
Takizawa, Y.
Kajino, F.
Engel, R.
Inoue, N.
Orleański, P.
Cafagna, F.
Yoshida, K.
Yonetoku, D.
Flamini, M.
Plebaniak, Z.
Saito, A.
Blanc, N.
Galeotti, P.
Rodríguez Frías, M. D.
Santiago Crúz, L.
Putis, M.
Schieler, H.
Hachisu, Y.
Nomoto, K.
Ricci, M.
Arai, Y.
Silva López, H. H.
Berlind, A. A.
Weiler, T. J.
Supanitsky, D.
Mernik, T.
Dupieux, M.
Fornaro, C.
Casolino, M.
Selmane, S.
Andreev, V.
del Peral, L.
Finco, D.
Shibata, T.
Kim, S.-W.
Tymieniecka, T.
Pennypacker, C.
Rusinov, I.
Lachaud, C.
Ferrarese, S.
Ikeda, D.
Karczmarczyk, J.
Chikawa, M.
Takami, H.
Marini, A.
Shirahama, T.
Belov, K.
Guzmán, A.
Tsunesada, Y.
Piraino, S.
Campana, D.
Prat, P.
Rodríguez, I.
Kaneko, I.
Dell’Oro, A.
Ebisuzaki, T.
Kim, J.-S.
Batsch, T.
Nava, R.
Rybczyński, M.
Szabelska, B.
von Ballmoos, P.
Baragatti, P.
Falk, S.
Ogio, S.
Murakami, T.
Capdevielle, J.-N.
Karadzhov, Y.
Sato, M.
Pastircak, B.
Vigorito, C.
Prieto, H.
Prévôt, G.
Tkachev, L.
Blümer, J.
Hernández Carretero, J.
Parizot, E.
López, F.
Allard, D.
Kleifges, M.
Takeda, M.
Tajima, T.
Modestino, G.
Yang, J.
Wada, S.
Katahira, K.
Sharakin, S.
Zuccaro Marchi, A.
Yashin, I. V.
Cellino, A.
Insolia, A.
Ohmori, H.
Maravilla, D.
Nagata, M.
Ikeda, H.
De Santis, C.
Blin-Bondil, S.
Csorna, S.
Napolitano, T.
Osteria, G.
Ronga, F.
Słomińska, K.
Kolev, D.
Di Martino, M.
Morozenko, V. S.
Błęcki, J.
Fang, K.
Jung, A.
Matev, R.
Roth, M.
Anzalone, A.
Kusenko, A.
Trillaud, F.
Wibig, T.
Yamamoto, T.
Blaksley, C.
Guarino, F.
Semikoz, D.
Connaughton, V.
Kawasaki, Y.
Zotov, M. Yu.
De Simone, N.
Catalano, C.
Mase, K.
Anchordoqui, L.
Kajino, T.
Uchihori, Y.
Unger, M.
Sánchez, S.
Suzuki, M.
Cremonini, R.
Fenu, F.
Lim, H.
Lee, J.
Kurihara, Y.
Perez Cano, S.
Giraudo, G.
Shimizu, H. M.
Yoshida, S.
Naumov, D.
Khrenov, B. A.
Monnier-Ragaigne, D.
Tokuno, H.
Cassardo, C.
Bayer, J.
Martinez, O.
Watts, J., Jr
Gorodetzky, P.
Crawford, H. J.
Wille, M.
Tsuno, K.
Sabau, M. D.
de Castro, A. J.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Science of atmospheric phenomena with JEM-EUSO
Autorzy:
Panasyuk, M. I.
Mot, B.
Garipov, G.
Keilhauer, B.
Sagawa, H.
Ebersoldt, A.
Kuznetsov, E.
Vankova, G.
Wilms, J.
Picozza, P.
Cordero, G.
Włodarczyk, Z.
Salazar, H.
Briggs, M. S.
Pierog, T.
Fujimoto, J.
Park, H. W.
Neronov, A.
Schanz, T.
Ogawa, T.
Geary, J.
Christl, M. J.
Segreto, A.
Dagoret-Campagne, S.
Bobik, P.
Bertaina, M.
Higashide, K.
Paul, T.
Harlov, B.
Park, I. H.
Vaduvescu, O.
Scotti, V.
Ave Pernas, M.
Kudela, K.
Maccarone, M. C.
Murakami, M. Nagano
Bellotti, R.
Roudil, G.
Catalano, G.
Dulucq, F.
Castellinic, G.
Serra, M.
Franceschi, A.
Itow, Y.
Peter, T.
Gonchar, M.
Masciantonio, G.
Gelmini, G.
Belenguer, T.
Judd, E. G.
Siemieniec-Oziębło, Grażyna
Tone, N.
Kawai, K.
Valdés-Galicia, J. F.
Yamamoto, Y.
Bechini, R.
Sarazin, F.
Yano, H.
Isgrò, F.
Biermann, P. L.
Reyes, M.
Tsenov, R.
Piotrowski, L. W.
Haungs, A.
Mizumoto, Y.
Weber, M.
Miyamoto, H.
Szabelski, J.
Kreykenbohm, I.
Asano, K.
Morales de los Ríos, J. A.
Fernández-Gómez, I.
Conti, L.
Biktemerova, S.
Tomida, T.
Lacombe, M.
Licandro, J.
Karus, M.
Shinozaki, K.
Tibolla, O.
Cline, D.
Bonamente, M.
Miyazaki, Y.
Ahmad, S.
Sáez-Cano, G.
Valore, L.
Sato, H.
Saprykin, O.
Nonaka, T.
Toscano, S.
Sledd, J.
Adams Jr, J. H.
Fukushima, M.
Sakaki, N.
Moretto, C.
Tajima, N.
Takahashi, Y.
Monaco, A.
Marcelli, L.
Briz, S.
Watanabe, J.
Pollini, A.
Vallania, P.
Caruso, R.
Barrillon, P.
Klimov, P. A.
Tajima, F.
Sugiyama, T.
Albert, J.-N.
De Donato, C.
Watanabe, S.
de la Taille, C.
Nagataki, S.
Santangelo, A.
Olinto, A. V.
Sanz Palomino, M.
Sobey, A.
Bogomilov, M.
Mannheim, K.
Wiencke, L.
Inoue, S.
Reardon, P.
Joven, E.
Nakamura, T.
Distratis, G.
Medina-Tanco, G.
Rothkaehl, H.
Sakata, M.
Villaseñor, L.
Young, R.
Bruno, A.
Tenzer, C.
Patzak, T.
González Alvarado, C.
Takizawa, Y.
Kajino, F.
Engel, R.
Inoue, N.
Orleański, P.
Cafagna, F.
Yoshida, K.
Yonetoku, D.
Flamini, M.
Plebaniak, Z.
Saito, A.
Blanc, N.
Galeotti, P.
Rodríguez Frías, M. D.
Santiago Crúz, L.
Putis, M.
Schieler, H.
Hachisu, Y.
Nomoto, K.
Ricci, M.
Arai, Y.
Silva López, H. H.
Berlind, A. A.
Weiler, T. J.
Supanitsky, D.
Mernik, T.
Dupieux, M.
Fornaro, C.
Casolino, M.
Selmane, S.
Andreev, V.
del Peral, L.
Finco, D.
Shibata, T.
Kim, S.-W.
Tymieniecka, T.
Pennypacker, C.
Rusinov, I.
Lachaud, C.
Ferrarese, S.
Ikeda, D.
Karczmarczyk, J.
Chikawa, M.
Takami, H.
Marini, A.
Shirahama, T.
Belov, K.
Guzmán, A.
Tsunesada, Y.
Piraino, S.
Campana, D.
Prat, P.
Rodríguez, I.
Słomiński, J.
Kaneko, I.
Dell’Oro, A.
Ebisuzaki, T.
Kim, J.-S.
Batsch, T.
Nava, R.
Rybczyński, M.
Szabelska, B.
von Ballmoos, P.
Baragatti, P.
Falk, S.
Ogio, S.
Murakami, T.
Capdevielle, J.-N.
Karadzhov, Y.
Sato, M.
Pastircak, B.
Vigorito, C.
Prieto, H.
Prévôt, G.
Tkachev, L.
Blümer, J.
Hernández Carretero, J.
Parizot, E.
López, F.
Allard, D.
Kleifges, M.
Takeda, M.
Tajima, T.
Modestino, G.
Yang, J.
Wada, S.
Katahira, K.
Sharakin, S.
Zuccaro Marchi, A.
Yashin, I. V.
Cellino, A.
Insolia, A.
Ohmori, H.
Maravilla, D.
Nagata, M.
Ikeda, H.
De Santis, C.
Blin-Bondil, S.
Csorna, S.
Napolitano, T.
Osteria, G.
Ronga, F.
Słomińska, K.
Kolev, D.
Di Martino, M.
Morozenko, V. S.
Błęcki, J.
Fang, K.
Jung, A.
Matev, R.
Roth, M.
Anzalone, A.
Kusenko, A.
Trillaud, F.
Wibig, T.
Yamamoto, T.
Blaksley, C.
Guarino, F.
Semikoz, D.
Connaughton, V.
Kawasaki, Y.
Zotov, M. Yu.
De Simone, N.
Catalano, C.
Mase, K.
Anchordoqui, L.
Kajino, T.
Uchihori, Y.
Unger, M.
Sánchez, S.
Suzuki, M.
Cremonini, R.
Fenu, F.
Lim, H.
Lee, J.
Kurihara, Y.
Perez Cano, S.
Giraudo, G.
Shimizu, H. M.
Yoshida, S.
Naumov, D.
Khrenov, B. A.
Monnier-Ragaigne, D.
Tokuno, H.
Cassardo, C.
Bayer, J.
Martinez, O.
Watts, J., Jr
Gorodetzky, P.
Crawford, H. J.
Wille, M.
Tsuno, K.
Sabau, M. D.
de Castro, A. J.
Opis:
The main goal of the JEM-EUSO experiment is the study of Ultra High Energy Cosmic Rays (UHECR, 10^{19}−10^{21} e V), but the method which will be used (detection of the secondary light emissions induced by cosmic rays in the atmosphere) allows to study other luminous phenomena. The UHECRs will be detected through the measurement of the emission in the range between 290 and 430 m, where some part of Transient Luminous Events (TLEs) emission also appears. This work discusses the possibility of using the JEM-EUSO Telescope to get new scientific results on TLEs. The high time resolution of this instrument allows to observe the evolution of TLEs with great precision just at the moment of their origin. The paper consists of four parts: review of the present knowledge on the TLE, presentation of the results of the simulations of the TLE images in the JEM-EUSO telescope, results of the Russian experiment Tatiana–2 and discussion of the possible progress achievable in this field with JEM-EUSO as well as possible cooperation with other space projects devoted to the study of TLE – TARANIS and ASIM. In atmospheric physics, the study of TLEs became one of the main physical subjects of interest after their discovery in 1989. In the years 1992 – 1994 detection was performed from satellite, aircraft and space shuttle and recently from the International Space Station. These events have short duration (milliseconds) and small scales (km to tens of km) and appear at altitudes 50 – 100 km. Their nature is still not clear and each new experimental data can be useful for a better understanding of these mysterious phenomena.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł

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