2009ApJ...695.1550S


Query : 2009ApJ...695.1550S

2009ApJ...695.1550S - Astrophys. J., 695, 1550-1558 (2009/April-3)

Detailed analysis of filamentary structure in the Weibel instability.

SUZUKI A. and SHIGEYAMA T.

Abstract (from CDS):

We present results of a 2D3V kinetic Vlasov simulation of the Weibel instability. The kinetic Vlasov simulation allows us to investigate the velocity distribution of dilute plasmas, in which the effect of collisions between particles is negligible, and has the advantage that the accuracy of the calculated velocity distribution does not depend on the density of plasmas at each point in the physical space. We succeed in reproducing some features of the Weibel instability shown by other simulations, for example, the exponentially growing phase, the saturation of the magnetic field strength, the formation of filamentary structure, and the coalescence of the filaments. Especially, we concentrate on the behavior of the filaments after the saturation of the magnetic field strength and find that there is a kind of quasi-equilibrium states before the coalescence occurs. Furthermore, it is found that an analytical solution for stationary states of the 2D3V Vlasov-Maxwell system can reproduce some dominant features of the quasi-equilibrium, e.g., the configuration of the magnetic field and the velocity distribution at each point. The analytical expression could give a plausible model for the transition layer of a collisionless shock where a strong magnetic field generated by the Weibel instability provides an effective dissipation process instead of collisions between particles.

Abstract Copyright: ∼

Journal keyword(s): instabilities - magnetic fields - 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 SNR G347.3-00.5 SNR 17 12 27 -39 41.2     12.27     ~ 761 1

Query : 2009ApJ...695.1550S

Basic data :
SNR G347.3-00.5 -- SuperNova Remnant
Other object types:
otypes_help
gam (2018A&A,1FGL,...), X (2022MNRAS,RX,...), SNR (2009BASI,SNR), BL? (2021MNRAS), V* (2012A&A), SR? (2014BASI)
ICRS coord. (ep=J2000) :
17 12 27.0 -39 41 12 [ ] D 2012ApJ...756....5L
FK4 coord. (ep=B1950 eq=1950) :
17 08 59.1 -39 37 38 [ ]
Gal coord. (ep=J2000) :
347.2695 -00.2569 [ ]
Angular size (arcmin):
65.0 55.0 ~ (Rad) D 2014BASI...42...47G
Fluxes (1) :
V 12.27 [0.07] C 2012A&A...548A..79A
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Identifiers (15) :
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SNR G347.3-00.5 4FGL J1713.5-3945e HESS J1713-397 TeV J1713-397
1FGL J1711.7-3944c 1FHL J1713.5-3951 RX J1713.7-3946 1WGA J1713.4-3946
2FGL J1712.4-3941 2FHL J1713.5-3945e 1RXS J171333.1-394544 [KRL2007b] 226
3FGL J1713.5-3945e 3FHL J1713.5-3945e SWIFT J1711.8-3935

References (761 between 1850 and 2026) (Total 761)
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

Distance : 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 : SNR G347.3-00.5

Link by name to the catalogue in VizieR :

1RXS J171333.1-394544

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