Turbulence, magnetic reconnection in turbulent fluids and energetic particle acceleration (2012)
- Authors:
- USP affiliated author: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- School: IAG
- DOI: 10.1007/s11214-012-9936-7
- Subjects: TURBULÊNCIA; MAGNETISMO; ACELERAÇÃO DE PARTÍCULAS; RAIOS CÓSMICOS
- Language: Inglês
- Imprenta:
- Place of publication: Rueil-Malmaison
- Date published: 2012
- Source:
- Título do periódico: Space Science Reviews
- ISSN: 0038-6308
- Volume/Número/Paginação/Ano: v. 173, p. 557-622, 2012
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
LAZARIAN, A; VLAHOS, L; KOWAL, G; et al. Turbulence, magnetic reconnection in turbulent fluids and energetic particle acceleration. Space Science Reviews, Rueil-Malmaison, v. 173, p. 557-622, 2012. Disponível em: < http://dx.doi.org/10.1007/s11214-012-9936-7 > DOI: 10.1007/s11214-012-9936-7. -
APA
Lazarian, A., Vlahos, L., Kowal, G., Yan, H., Beresnyak, A., & Dal Pino, E. M. de G. (2012). Turbulence, magnetic reconnection in turbulent fluids and energetic particle acceleration. Space Science Reviews, 173, 557-622. doi:10.1007/s11214-012-9936-7 -
NLM
Lazarian A, Vlahos L, Kowal G, Yan H, Beresnyak A, Dal Pino EM de G. Turbulence, magnetic reconnection in turbulent fluids and energetic particle acceleration [Internet]. Space Science Reviews. 2012 ; 173 557-622.Available from: http://dx.doi.org/10.1007/s11214-012-9936-7 -
Vancouver
Lazarian A, Vlahos L, Kowal G, Yan H, Beresnyak A, Dal Pino EM de G. Turbulence, magnetic reconnection in turbulent fluids and energetic particle acceleration [Internet]. Space Science Reviews. 2012 ; 173 557-622.Available from: http://dx.doi.org/10.1007/s11214-012-9936-7 - Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
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Informações sobre o DOI: 10.1007/s11214-012-9936-7 (Fonte: oaDOI API)
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