Search Results - "Yurkin, Y Y"

PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra by Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Gillard, W., Grishantseva, L., Jerse, G., Karelin, A. V., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Malvezzi, V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, L., Sarkar, R., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Wu, J., Zampa, G., Zampa, N., Zverev, V. G.

“…Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the…”
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Time Dependence of the Flux of Helium Nuclei in Cosmic Rays Measured by the PAMELA Experiment between 2006 July and 2009 December by Marcelli, N., Boezio, M., Lenni, A., Menn, W., Munini, R., Aslam, O. P. M., Bisschoff, D., Ngobeni, M. D., Potgieter, M. S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Santis, C., Galper, A. M., Koldashov, S. V., Koldobskiy, S., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Mergè, M., Mocchiutti, E., Monaco, A., Mori, N., Mikhailov, V. V., Osteria, G., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sotgiu, A., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N.

“…Precise time-dependent measurements of the Z = 2 component in the cosmic radiation provide crucial information about the propagation of charged particles…”
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Evidence of Energy and Charge Sign Dependence of the Recovery Time for the 2006 December Forbush Event Measured by the PAMELA Experiment by Munini, R., Boezio, M., Bruno, A., Christian, E. C., Nolfo, G. A. de, Felice, V. Di, Martucci, M., Merge', M., Richardson, I. G., Ryan, J. M., Stochaj, S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bongi, M., Bonvicini, V., Bottai, S., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., Santis, C. De, Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Osteria, G., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Potgieter, M. S.

“…New results on the short-term galactic cosmic-ray (GCR) intensity variation (Forbish decrease) in 2006 December measured by the PAMELA instrument are…”
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Helium Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24 by Marcelli, N., Boezio, M., Lenni, A., Menn, W., Munini, R., Aslam, O. P. M., Bisschoff, D., Ngobeni, M. D., Potgieter, M. S., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Santis, C., Galper, A. M., Koldashov, S. V., Koldobskiy, S., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Mergè, M., Mocchiutti, E., Monaco, A., Mori, N., Mikhailov, V. V., Osteria, G., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sotgiu, A., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N.

“…Abstract Time-dependent energy spectra of galactic cosmic rays (GCRs) carry fundamental information regarding their origin and propagation. When observed at…”
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East–West Proton Flux Anisotropy Observed with the PAMELA Mission by Bruno, A., Martucci, M., Cafagna, F. S., Sparvoli, R., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Campana, D., Carlson, P., Casolino, M., Castellini, G., Santis, C. De, Galper, A. M., Koldashov, S. V., Koldobskiy, S., Kvashnin, A. N., Lenni, A., Leonov, A. A., Malakhov, V. V., Marcelli, L., Marcelli, N., Mayorov, A. G., Menn, W., Mergè, M., Mocchiutti, E., Monaco, A., Mori, N., Mikhailov, V. V., Munini, R., Osteria, G., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sotgiu, A., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N.

“…We present a study of the east–west anisotropy of trapped-proton fluxes in low-Earth orbit based on the measurements of the Payload for Antimatter Matter…”
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Study of Forbush Decrease Recovery Times by the Payload for Antimatter Matter Exploration and Light-Nuclei Astrophysics (PAMELA) Experiment by Lagoida, I. A., Voronov, S. A., Mikhailov, V. V., Boezio, M., Munini, R., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Bogomolov, E. A., Bonvicini, V., Cafagna, F., Campana, D., Casolino, M., Galper, A. M., Koldobskiy, S. A., Kvashnin, A. N., Lenni, A., Leonov, A. N., Malakhov, V., Marcelli, L., Marcelli, N., Martucci, M., Mayorov, A., Mergè, M., Mocchiutti, E., Monaco, A., Panico, B., Picozza, P., Ricci, M., Ricciarini, S. B., Rodenko, S., Sotgiu, A., Sparvoli, R., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Yurkin, Y. T., Zampa, G., Zampa, N.

“…A Forbush decrease (FD) is a sudden drop of cosmic-ray intensity arising as an effect of coronal mass ejection (CME) propagation in interplanetary space. The…”
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Lithium and Beryllium Isotopes with the PAMELA Experiment by Menn, W., Bogomolov, E. A., Simon, M., Vasilyev, G., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Mergè, M, Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N.

“…The cosmic ray (CR) lithium and beryllium (6Li, 7Li, 7Be, 9Be, 10Be) isotopic composition has been measured with the satellite-borne experiment PAMELA, which…”
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Cosmic-ray positron energy spectrum measured by PAMELA by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Bianco, A, Boezio, M, Bogomolov, E A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, A M, Karelin, A V, Koldashov, S V, Koldobskiy, S A, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A G, Menn, W, Mergé, M, Mikhailov, V V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, S B, Rossetto, L, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stochaj, S J, Stockton, J C, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G I, Voronov, S A, Yurkin, Y T, Zampa, G, Zampa, N, Zverev, V G

“…Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of…”
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PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Boezio, M, Bogomolov, E A, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Consiglio, L, De Pascale, M P, De Santis, C, De Simone, N, Di Felice, V, Galper, A M, Gillard, W, Grishantseva, L, Hofverberg, P, Jerse, G, Karelin, A V, Koldashov, S V, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malvezzi, V, Marcelli, L, Mayorov, A G, Menn, W, Mikhailov, V V, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, S B, Rossetto, L, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S A, Wu, J, Yurkin, Y T, Zampa, G, Zampa, N, Zverev, V G

“…The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio which…”
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Cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Boezio, M, Bogomolov, E A, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Consiglio, L, De Pascale, M P, De Santis, C, De Simone, N, Di Felice, V, Galper, A M, Gillard, W, Grishantseva, L, Jerse, G, Karelin, A V, Koldashov, S V, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malakhov, V, Malvezzi, V, Marcelli, L, Mayorov, A G, Menn, W, Mikhailov, V V, Mocchiutti, E, Monaco, A, Mori, N, Nikonov, N, Osteria, G, Palma, F, Papini, P, Pearce, M, Picozza, P, Pizzolotto, C, Ricci, M, Ricciarini, S B, Rossetto, L, Sarkar, R, Simon, M, Sparvoli, R, Spillantini, P, Stochaj, S J, Stockton, J C, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S A, Wu, J, Yurkin, Y T, Zampa, G, Zampa, N, Zverev, V G

“…Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the…”
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New upper limit on strange quark matter abundance in cosmic rays with the PAMELA space experiment by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Boezio, M, Bogomolov, E A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, A M, Karelin, A V, Koldashov, S V, Koldobskiy, S, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A G, Menn, W, Mergè, M, Mikhailov, V V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S A, Yurkin, Y T, Zampa, G, Zampa, N

“…In this work we present results of a direct search for strange quark matter (SQM) in cosmic rays with the PAMELA space spectrometer. If this state of matter…”
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Time Dependence of the Electron and Positron Components of the Cosmic Radiation Measured by the PAMELA Experiment between July 2006 and December 2015 by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Boezio, M, Bogomolov, E A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Santis, C, Di Felice, V, Galper, A M, Karelin, A V, Koldashov, S V, Koldobskiy, S A, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A G, Menn, W, Mergé, M, Mikhailov, V V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S B, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G I, Voronov, S A, Yurkin, Y T, Zampa, G, Zampa, N, Potgieter, M S, Vos, E E

“…Cosmic-ray electrons and positrons are a unique probe of the propagation of cosmic rays as well as of the nature and distribution of particle sources in our…”
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New measurement of the antiproton-to-proton flux ratio up to 100 GeV in the cosmic radiation by Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Boezio, M, Bogomolov, E A, Bonechi, L, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Pascale, M P, De Rosa, G, Fedele, D, Galper, A M, Grishantseva, L, Hofverberg, P, Leonov, A, Koldashov, S V, Krutkov, S Y, Kvashnin, A N, Malvezzi, V, Marcelli, L, Menn, W, Mikhailov, V V, Minori, M, Mocchiutti, E, Nagni, M, Orsi, S, Osteria, G, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S B, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y I, Taddei, E, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S A, Yurkin, Y T, Zampa, G, Zampa, N, Zverev, V G

“…A new measurement of the cosmic-ray antiproton-to-proton flux ratio between 1 and 100 GeV is presented. The results were obtained with the PAMELA experiment,…”
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Lithium and Beryllium Isotopes in the PAMELA Experiment by Bogomolov, E. A., Vasilyev, G. I., Menn, W., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldobskiy, S. A., Lagoida, I. A., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Yurkin, Y. T.

“…The isotopic composition of Li and Be nuclei in the 1–5 GV range of rigidities (nuclear energies of 0.1–1.5 GeV/nucleon) is analyzed using PAMELA flight data…”
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PAMELA and indirect dark matter searches by Boezio, M, Pearce, M, Picozza, P, Sparvoli, R, Spillantini, P, Adriani, O, Barbarino, G C, Bazilevskaya, G A, Bellotti, R, Bogomolov, E A, Bonechi, L, Bongi, M, Bonvicini, V, Borisov, S, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, Consiglio, L, De Pascale, M P, Santis, C De, Simone, N De, Felice, V Di, Galper, A M, Grishantseva, L, Gillard, W, Hofverberg, P, Koldashov, S V, Krutkov, S Y, Kvashnin, A N, Leonov, A, Malvezzi, V, Marcelli, L, Menn, W, Mikhailov, V V, Mocchiutti, E, Mori, N, Nikonov, N, Osteria, G, Papini, P, Ricci, M, Ricciarini, S B, Simon, M, Stozhkov, Y I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S A, Yurkin, Y T, Zampa, G, Zampa, N, Zverev, V G

“…We present a review of the experimental results obtained by PAMELA in measuring the (p, (p) over bar ) and e(+/-) abundance in cosmic rays. In this context, we…”
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Evaluation of State of Ultrasonic Medical Diagnostic Devices in Hospitals and Clinics of Moscow Health Care Department by Gromov, A. I., Osipov, L. V., Yurkin, Y. Y., Burashov, V. V., Soldatov, I. V.

“…The goal of this work was to assess the state of ultrasonic medical diagnostic equipment in hospitals and clinics of the Department of Health Care of Moscow…”
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Trapped Positrons and Electrons in the Inner Radiation Belt According to Data of the PAMELA Experiment by Mikhailov, V. V., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Bogomolov, E. A., Boezio, M., Bonvicini, V., Bongi, M., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Galper, A. M., De Santis, C., Di Felice, V., Zampa, G., Zampa, N., Casolino, M., Campana, D., Karelin, A. V., Carlson, P., Castellini, G., Cafagna, F., Kvashnin, A. A., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Leonov, A. A., Mayorov, A. G., Malakhov, V. V., Martucci, M., Marcelli, L., Menn, W., Merge, M., Mikhailova, Yu. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Picozza, P., Pearce, M., Ricci, M., Ricciarini, S. B., Runtso, M. F., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Yurkin, Y. T.

“…Measurements of secondary-electron and secondary-positron fluxes below the geomagnetic cutoff in near-Earth space were performed by means of the PAMELA…”
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Time dependence of the helium flux measured by PAMELA by Marcelli, N., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Santis, C., Di Felice, V., Galper, A. M., Karelin, A.V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Potgieter, M. S., Aslam, O. P. M., Bisschoff, D.

“…Precision measurements of the Z = 2 component in cosmic radiation provide crucial information about the origin and propagation of the second most abundant…”
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Evaluation of the condition of ultrasonic medical diagnostic devices in hospitals and dinics of the Moscow Health Care Department by Gromov, A I, Osipov, L V, Yurkin, Y Y, Burashov, V V, Solatov, I V

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Characteristics of the GAMMA-400 gamma-ray telescope for searching for dark matter signatures by Galper, A. M., Adriani, O., Aptekar, R. L., Arkhangelskaja, I. V., Arkhangelskiy, A. I., Boezio, M., Bonvicini, V., Boyarchuk, K. A., Vacchi, A., Vannuccini, E., Gusakov, Yu. V., Zampa, N., Zverev, V. G., Zirakashvili, V. N., Kaplin, V. A., Kachanov, V. A., Leonov, A. A., Longo, F., Mazets, E. P., Maestro, P., Marrocchesi, P., Mereminskiy, I. A., Mikhailov, V. V., Moiseev, A. A., Mocchiutti, E., Mori, N., Moskalenko, I. V., Naumov, P. Yu, Papini, P., Picozza, P., Rodin, V. G., Runtso, M. F., Sparvoli, R., Spillantini, P., Suchkov, S. I., Tavani, M., Topchiev, N. P., Fradkin, M. I., Kheymits, M. D., Yurkin, Y. T.

“…The GAMMA-400 gamma-ray telescope currently under development is designed to measure fluxes of gamma rays and electron-positron cosmic-ray components, which…”
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