2015ApJ...802..115K


Query : 2015ApJ...802..115K

2015ApJ...802..115K - Astrophys. J., 802, 115 (2015/April-1)

Particle acceleration and wave excitation in quasi-parallel high-mach-number collisionless shocks: particle-in-cell simulation.

KATO T.N.

Abstract (from CDS):

We herein investigate shock formation and particle acceleration processes for both protons and electrons in a quasi-parallel high-Mach-number collisionless shock through a long-term, large-scale, particle-in-cell simulation. We show that both protons and electrons are accelerated in the shock and that these accelerated particles generate large-amplitude Alfvénic waves in the upstream region of the shock. After the upstream waves have grown sufficiently, the local structure of the collisionless shock becomes substantially similar to that of a quasi-perpendicular shock due to the large transverse magnetic field of the waves. A fraction of protons are accelerated in the shock with a power-law-like energy distribution. The rate of proton injection to the acceleration process is approximately constant, and in the injection process, the phase-trapping mechanism for the protons by the upstream waves can play an important role. The dominant acceleration process is a Fermi-like process through repeated shock crossings of the protons. This process is a ''fast'' process in the sense that the time required for most of the accelerated protons to complete one cycle of the acceleration process is much shorter than the diffusion time. A fraction of the electrons are also accelerated by the same mechanism, and have a power-law-like energy distribution. However, the injection does not enter a steady state during the simulation, which may be related to the intermittent activity of the upstream waves. Upstream of the shock, a fraction of the electrons are pre-accelerated before reaching the shock, which may contribute to steady electron injection at a later time.

Abstract Copyright: ∼

Journal keyword(s): acceleration of particles - cosmic rays - ISM: supernova remnants - methods: numerical - plasmas - shock waves

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1

Query : 2015ApJ...802..115K

Basic data :
NAME Lupus SN -- SuperNova Remnant
Other object types:
otypes_help
X (1E,1ES,...), SNR (2009BASI,AJG,...), Rad (GRS,MRC,...), SN* (SN), gam (TeV)
ICRS coord. (ep=J2000) :
15 02 22.1 -42 05 49 [ 3000 3000 90 ] D 1990PKS...C......0W
FK4 coord. (ep=B1950 eq=1950) :
14 59 05.6 -41 54 02 [ 3000 3000 90 ]
Gal coord. (ep=J2000) :
327.4109 +14.4674 [ 3000 3000 90 ]
Angular size (arcmin):
30.0 30.0 90 (Rad) D 2014BASI...42...47G
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Identifiers (24) :
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NAME Lupus SN H 1506-42 PKS 1459-419 SN 1006
AJG 37 KOHX 1 PKS J1502-4205 TeV J1502-419
1E 1459.6-4146 1M 1457-416 SNR G327.6+14.6 2U 1440-39
1ES 1500-41.5 MRC 1459-417 SNR G327.6+14.5 3U 1439-39
GRS G327.60 +14.60 MSH 14-4-15 SN 1006A 4U 1458-41
1H 1458-416 PKS 1459-41 SN 1016 XSS J15031-4149

References (1407 between 1850 and 2026) (Total 1407)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

SpT : 1   

   

Observing logs
XMM : 9   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : NAME Lupus SN

Link by name to the catalogue in VizieR :

PKS 1459-41 PKS 1459-419 PKS J1502-4205

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