Published February 2012
| Version v1
Journal article
A 3D Monte Carlo code for the modeling of plasma dynamics and beam formation mechanism in electron cyclotron resonance ion sources
- 1. INFN-Laboratori Nazionali del Sud, via S. Sofia 62, 95123 Catania (Italy)
Description
The code here presented is the first part of a Monte Carlo (MC) self-consistent 3D plasma simulator. It is yet able to solve the equation of motion for thousands of independent charged particles. The procedure allows to understand the consequences of each phenomenon introduced in the evolution steps of the code. MC random selection of starting parameters is used for each particles; the environmental conditions enclosed in the simulation are ECRIS magnetic field, resonant electromagnetic wave, initial plasma density distribution and MC calculation of Spitzer collision. The results of the first simulations explain some typical effects as the hollow beam formation and the main plasma deconfinement mechanism.
Additional details
Identifiers
- DOI
- 10.1063/1.3670341;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 83
- Journal Issue
- 2
- Journal Page Range
- p. 02A330-02A330.3
- ISSN
- 0034-6748
- CODEN
- RSINAK
Conference
- Title
- 14. international conference on ion sources
- Acronym
- ICIS 2011
- Dates
- 12-16 Sep 2011
- Place
- Giardini-Naxos, Sicily (Italy)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44023057
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BEAM-PLASMA SYSTEMS; CHARGED PARTICLES; ECR ION SOURCES; ELECTROMAGNETIC RADIATION; EQUATIONS OF MOTION; MAGNETIC FIELDS; MONTE CARLO METHOD; PLASMA CONFINEMENT; PLASMA DENSITY; PLASMA SIMULATION; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- CALCULATION METHODS; CONFINEMENT; DIFFERENTIAL EQUATIONS; EQUATIONS; ION SOURCES; PARTIAL DIFFERENTIAL EQUATIONS; RADIATIONS; SIMULATION
Optional Information
- Notes
- (c) 2012 American Institute of Physics