We describe a parallel version of our high-order-accuracy particle-mesh code for the simulation of collisionless protoplanetary disks. We use this code to carry out a massively parallel, two-dimensional, time-dependent, numerical simulation, which includes dust particles, to study the potential role
β¦ LIBER β¦
Dynamics of charged dust particles in protoplanetary discs
β Scribed by Mohsen Shadmehri
- Publisher
- Springer Netherlands
- Year
- 2008
- Tongue
- English
- Weight
- 327 KB
- Volume
- 314
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Dust Dynamics in Protoplanetary Disks: P
β
Carlos de la Fuente Marcos; Pierre Barge; RaΓΊl de la Fuente Marcos
π
Article
π
2002
π
Elsevier Science
π
English
β 277 KB
Dynamics of charged particles in optical
β
A.I. Dzergatch; V.A. Kuzmin; S.V. Vinogradov
π
Article
π
2006
π
Elsevier Science
π
English
β 422 KB
Charge measurement of dust particles in
β
J.B. Gajewski; A. Szaynok
π
Article
π
1981
π
Elsevier Science
π
French
β 275 KB
Abnormal Kinetic Energy of Charged Dust
β
G. Norman; V. Stegailov; A. Timofeev
π
Article
π
2010
π
John Wiley and Sons
π
English
β 127 KB
π 1 views
## Abstract A mechanism of the increase of the average kinetic energy of charged dust particles in gas discharge plasmas is suggested. Particle charge fluctuation is the reason for the appearance of forced resonance, which heats vertical oscillations. The energy transfer from vertical oscillations
The ionization fraction in Ξ± models of p
β
SΓ©bastien Fromang; Caroline Terquem; Steven A. Balbus
π
Article
π
2002
π
John Wiley and Sons
π
English
β 298 KB
Destruction of protoplanetary discs in t
β
Aylwyn Scally; Cathie Clarke
π
Article
π
2001
π
John Wiley and Sons
π
English
β 402 KB