SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(Koldashov S. V.)
 

Search: WFRF:(Koldashov S. V.) > Pamela's measuremen...

Pamela's measurements of magnetospheric effects on high-energy solar particles

Adriani, O. (author)
Barbarino, G. C. (author)
Bazilevskaya, G. A. (author)
show more...
Bellotti, R. (author)
Boezio, M. (author)
Bogomolov, E. A. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Bottai, S. (author)
Bravar, U. (author)
Bruno, A. (author)
Cafagna, F. (author)
Campana, D. (author)
Carbone, R. (author)
Carlson, Per (author)
KTH,Partikel- och astropartikelfysik
Casolino, M. (author)
Castellini, G. (author)
Christian, E. R. (author)
De Donato, C. (author)
de Nolfo, G. A. (author)
De Santis, C. (author)
De Simone, N. (author)
Di Felice, V. (author)
Formato, V. (author)
Galper, A. M. (author)
Karelin, A. V. (author)
Koldashov, S. V. (author)
Koldobskiy, S. (author)
Krutkov, S. Y. (author)
Kvashnin, A. N. (author)
Lee, M. (author)
Leonov, A. (author)
Malakhov, V. (author)
Marcelli, L. (author)
Martucci, M. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Merge, M. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Monaco, A. (author)
Mori, N. (author)
Munini, R. (author)
Osteria, G. (author)
Palma, F. (author)
Panico, B. (author)
Papini, P. (author)
Pearce, Mark (author)
KTH,Partikel- och astropartikelfysik
Picozza, P. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Ryan, J. M. (author)
Sarkar, R. (author)
Scotti, V. (author)
Simon, M. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stochaj, S. (author)
Stozhkov, Y. I. (author)
Thakur, N. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. I. (author)
Voronov, S. A. (author)
Yurkin, Y. T. (author)
Zampa, G. (author)
Zampa, N. (author)
show less...
 (creator_code:org_t)
2015
2015
English.
In: Astrophysical Journal Letters. - 2041-8205 .- 2041-8213. ; 801:1
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • The nature of particle acceleration at the Sun, whether through flare reconnection processes or through shocks driven by coronal mass ejections, is still under scrutiny despite decades of research. The measured properties of solar energetic particles (SEPs) have long been modeled in different particle-acceleration scenarios. The challenge has been to disentangle the effects of transport from those of acceleration. The Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) instrument enables unique observations of SEPs including the composition and angular distribution of the particles about the magnetic field, i.e., pitch angle distribution, over a broad energy range (>80 MeV)-bridging a critical gap between space-based and ground-based measurements. We present high-energy SEP data from PAMELA acquired during the 2012 May 17 SEP event. These data exhibit differential anisotropies and thus transport features over the instrument rigidity range. SEP protons exhibit two distinct pitch angle distributions: a low-energy population that extends to 90 degrees and a population that is beamed at high energies (>1 GeV), consistent with neutron monitor measurements. To explain a low-energy SEP population that exhibits significant scattering or redistribution accompanied by a high-energy population that reaches the Earth relatively unaffected by dispersive transport effects, we postulate that the scattering or redistribution takes place locally. We believe that these are the first comprehensive measurements of the effects of solar energetic particle transport in the Earth's magnetosheath.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Earth
Sun: coronal mass ejections (CMEs)
Sun: flares
Sun: heliosphere
Sun: particle emission

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view