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Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24
- Source :
- The astrophysical journal. Letters, 854 (2018). doi:10.3847/2041-8213/aaa9b2, info:cnr-pdr/source/autori:Martucci M.; Munini R.; Boezio M.; Felice V.D.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Bongi M.; Bonvicini V.; Bottai S.; Bruno A.; Cafagna F.; Campana D.; Carlson P.; Casolino M.; Castellini G.; Santis C.D.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobskiy S.; Krutkov S.Y.; Kvashnin A.N.; Leonov A.; Malakhov V.; Marcelli L.; Marcelli N.; Mayorov A.G.; Menn W.; Merge M.; 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.; Raath J.L./titolo:Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24/doi:10.3847%2F2041-8213%2Faaa9b2/rivista:The astrophysical journal. Letters (Print)/anno:2018/pagina_da:/pagina_a:/intervallo_pagine:/volume:854
- Publication Year :
- 2018
- Publisher :
- IOP Publishing, Bristol , Regno Unito, 2018.
-
Abstract
- Precise measurements of the time-dependent intensity of the low-energy (
- Subjects :
- Astroparticle physics
Physics
astroparticle physics
cosmic rays
Sun: heliosphere
Astronomy and Astrophysics
Space and Planetary Science
010504 meteorology & atmospheric sciences
Proton
Astrophysics::High Energy Astrophysical Phenomena
Settore FIS/04
astroparticle physic
Cosmic ray
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
Solar cycle 24
01 natural sciences
0103 physical sciences
Physics::Space Physics
010303 astronomy & astrophysics
cosmic ray
Intensity (heat transfer)
0105 earth and related environmental sciences
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- The astrophysical journal. Letters, 854 (2018). doi:10.3847/2041-8213/aaa9b2, info:cnr-pdr/source/autori:Martucci M.; Munini R.; Boezio M.; Felice V.D.; Adriani O.; Barbarino G.C.; Bazilevskaya G.A.; Bellotti R.; Bongi M.; Bonvicini V.; Bottai S.; Bruno A.; Cafagna F.; Campana D.; Carlson P.; Casolino M.; Castellini G.; Santis C.D.; Galper A.M.; Karelin A.V.; Koldashov S.V.; Koldobskiy S.; Krutkov S.Y.; Kvashnin A.N.; Leonov A.; Malakhov V.; Marcelli L.; Marcelli N.; Mayorov A.G.; Menn W.; Merge M.; 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.; Raath J.L./titolo:Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24/doi:10.3847%2F2041-8213%2Faaa9b2/rivista:The astrophysical journal. Letters (Print)/anno:2018/pagina_da:/pagina_a:/intervallo_pagine:/volume:854
- Accession number :
- edsair.doi.dedup.....405ef7d9dfc0cdb35bf5a120e671284f
- Full Text :
- https://doi.org/10.3847/2041-8213/aaa9b2