Comparing Long-Duration Gamma-Ray Flares and High-Energy Solar Energetic Particles

Autor: de Nolfo, G. A., Bruno, A., Ryan, J. M., Dalla, S., Giacalone, J., Richardson, I. G., Christian, E. R., Stochaj, S. J., Bazilevskaya, G. A., Boezio, M., Martucci, M., Mikhailov, V. V., Munini, R.

Publikováno v: de Nolfo et al. 2019, ApJ 879 90

Little is known about the origin of the high-energy and sustained emission from solar Long-Duration Gamma-Ray Flares (LDGRFs), identified with the Compton Gamma Ray Observatory (CGRO), the Solar Maximum Mission (SMM), and now Fermi. Though Fermi/Larg

Externí odkaz: http://arxiv.org/abs/1905.12878

Cosmic-Ray Positron Identification with the PAMELA experiment

Autor: 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 Santis, C., De Pascale, M. P., De Donato, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krut'kov, S. Yu., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge`, 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., Simon, M., Scotti, V., Sparvoli, R., Spillantini, P., Stochaj, S. J., Stockton, J. C., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G.

The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range. One of PAMELA's main goal is the study of the antimatter component of cosmic rays. The experiment, housed on board the Russian satellit

Externí odkaz: http://arxiv.org/abs/1306.2198

The Cosmic-Ray Proton and Helium Spectra measured with the CAPRICE98 balloon experiment

Autor: Boezio, M., Bonvicini, V., Schiavon, P., Vacchi, A., Zampa, N., Bergstroem, D., Carlson, P., Francke, T., Hansen, P., Mocchiutti, E., Suffert, M., Hof, M., Kremer, J., Menn, W., Simon, M., Ambriola, M., Bellotti, R., Cafagna, F., Ciacio, F., Circella, M., De Marzo, C. N., Finetti, N., Papini, P., Piccardi, S., Spillantini, P., Vannuccini, E., Bartalucci, S., Ricci, M., Casolino, M., De Pascale, M. P., Morselli, A., Picozza, P., Sparvoli, R., Mitchell, J. W., Ormes, J. F., Stephens, S. A., Streitmatter, R. E., Bravar, U., Stochaj, S. J.

Publikováno v: Astropart.Phys. 19 (2003) 583-604

A new measurement of the primary cosmic-ray proton and helium fluxes from 3 to 350 GeV was carried out by the balloon-borne CAPRICE experiment in 1998. This experimental setup combines different detector techniques and has excellent particle discrimi

Externí odkaz: http://arxiv.org/abs/astro-ph/0212253

Cosmic-Ray Positron Energy Spectrum Measured by PAMELA

Autor: PAMELA Collaboration, 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., Merge', 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.

Publikováno v: Physical review letters (CD-ROM) 111 (2013). doi:10.1103/PhysRevLett.111.081102
info:cnr-pdr/source/autori:Adriani, O., Barbarino, G.C., Bazilevskaya, G.A., Bellotti, R., Bianco, Castellini, G.,Ricciarini, S.B., et al./titolo:Cosmic-ray positron energy spectrum measured by PAMELA/doi:10.1103%2FPhysRevLett.111.081102/rivista:Physical review letters (CD-ROM)/anno:2013/pagina_da:/pagina_a:/intervallo_pagine:/volume:111

Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e55a6306687fc719f6f46e9e4b16169
http://hdl.handle.net/11390/1125110

New measurements of the flux of atmospheric muons

Autor: Boezio, M., Carlson, P., Francke, T., Weber, N., Suffert, M., Hof, M., Menn, W., Simon, M., Stephens, S. A., Bellotti, R., Cafagna, F., Castellano, M., Circella, M., De Marzo, C., Grimani, Catia, Finetti, N., Papini, P., Piccardi, S., Spillantini, P., Ricci, M., Casolino, M., De Pascale, M. P., Morselli, A., Picozza, P., Sparvoli, R., Barbiellini, G., Bravar, U., Schiavon, P., Vacchi, A., Zampa, N., Mitchell, J. W., Ormes, J. F., Streitmatter, R. E., Golden, R. L., Stochaj, S. J.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3656::318ca72620c3e12cc9b1f0c37c3b907e
https://hdl.handle.net/11576/1877758