Show simple item record
Author | dc.contributor.author | Ley, Francisco | |
Author | dc.contributor.author | Riquelme, Mario | |
Author | dc.contributor.author | Sironi, Lorenzo | |
Author | dc.contributor.author | Verscharen, Daniel | |
Author | dc.contributor.author | Sandoval, Astor | |
Admission date | dc.date.accessioned | 2019-10-11T17:30:12Z | |
Available date | dc.date.available | 2019-10-11T17:30:12Z | |
Publication date | dc.date.issued | 2019 | |
Cita de ítem | dc.identifier.citation | Astrophysical Journal, Volumen 880, Issue 2, 2019, | |
Identifier | dc.identifier.issn | 15384357 | |
Identifier | dc.identifier.issn | 0004637X | |
Identifier | dc.identifier.other | 10.3847/1538-4357/ab2592 | |
Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/171289 | |
Abstract | dc.description.abstract | © 2019 Institute of Physics Publishing. All rights reserved.Using 1D and 2D particle-in-cell simulations of a plasma with a growing magnetic field B, we show that ions can be stochastically accelerated by the ion-cyclotron (IC) instability. As B grows, an ion pressure anisotropy p⊥, i ≥ p∥, i arises due to the adiabatic invariance of the ion magnetic moment (p∥, i and p⊥, i are the ion pressures parallel and perpendicular to B). When initially βi = 0.5 (bi ≡ 8πpi |B|2, where pi is the ion isotropic pressure), the pressure anisotropy is limited mainly by inelastic pitch-angle scattering provided by the IC instability, which in turn produces a nonthermal tail in the ion energy spectrum. After B is amplified by a factor of ∼2.7, this tail can be approximated as a power law of index ∼3.4 plus two nonthermal bumps and accounts for 2%-3% of the ions and ∼18% of their kinetic energy. On the contrary, when initially β i = 2, the ion scattering is dominated by the mirror instability, and the ac | |
Lenguage | dc.language.iso | en | |
Publisher | dc.publisher | Institute of Physics Publishing | |
Type of license | dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Chile | |
Link to License | dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
Source | dc.source | Astrophysical Journal | |
Keywords | dc.subject | accretion, accretion disks | |
Keywords | dc.subject | instabilities | |
Keywords | dc.subject | plasmas | |
Título | dc.title | Stochastic Ion Acceleration by the Ion-cyclotron Instability in a Growing Magnetic Field | |
Document type | dc.type | Artículo de revista | |
dcterms.accessRights | dcterms.accessRights | Acceso Abierto | |
Cataloguer | uchile.catalogador | SCOPUS | |
Indexation | uchile.index | Artículo de publicación SCOPUS | |
uchile.cosecha | uchile.cosecha | SI | |
Files in this item
- Name:
- Ley_2019_ApJ_880_100.pdf
- Size:
- 2.321Mb
- Format:
- PDF
This item appears in the following Collection(s)
Show simple item record
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile