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A publicação pode ser exportada nos seguintes formatos: referência da APA (American Psychological Association), referência do IEEE (Institute of Electrical and Electronics Engineers), BibTeX e RIS.

Exportar Referência (APA) 
Stockem, A., Bret, A., Fonseca, R. A. & Silva, L. O. (2015). Shock formation in electron–ion plasmas: mechanism and timing. Astrophysical Journal Letters. 803 (2)
Exportar Referência (IEEE) 
A. Stockem et al.,  "Shock formation in electron–ion plasmas: mechanism and timing", in Astrophysical Journal Letters, vol. 803, no. 2, 2015
Exportar BibTeX 
@article{stockem2015_1766315341771,
	author = "Stockem, A. and Bret, A. and Fonseca, R. A. and Silva, L. O.",
	title = "Shock formation in electron–ion plasmas: mechanism and timing",
	journal = "Astrophysical Journal Letters",
	year = "2015",
	volume = "803",
	number = "2",
	doi = "10.1088/2041-8205/803/2/L29",
	url = "http://stacks.iop.org/2041-8205/803/i=2/a=L29?key=crossref.4bb8edd6ca2736549da9bd51a9af49a2"
}
Exportar RIS 
TY  - JOUR
TI  - Shock formation in electron–ion plasmas: mechanism and timing
T2  - Astrophysical Journal Letters
VL  - 803
IS  - 2
AU  - Stockem, A.
AU  - Bret, A.
AU  - Fonseca, R. A.
AU  - Silva, L. O.
PY  - 2015
SN  - 2041-8205
DO  - 10.1088/2041-8205/803/2/L29
UR  - http://stacks.iop.org/2041-8205/803/i=2/a=L29?key=crossref.4bb8edd6ca2736549da9bd51a9af49a2
AB  - We analyze the full shock formation process in electron-ion plasmas in theory and simulations. It is accepted that electromagnetic shocks in initially unmagnetized relativistic plasmas are triggered by filamentation instability. However, the transition from the first unstable phase to the quasi-steady shock is still missing. We derive a theoretical model for the shock formation time, taking into account filament merging in the nonlinear phase of the filamentation instability. This process is much slower than in electron-positron pair shocks, and so the shock formation is longer by a factor proportional to root m(i)/m(e) ln (m(i)/m(e)).
ER  -