http://www.cnr.it/ontology/cnr/individuo/prodotto/ID81188
SPECE: A Code for Electron Cyclotron Emission in Tokamaks (Contributo in atti di convegno)
- Type
- Label
- SPECE: A Code for Electron Cyclotron Emission in Tokamaks (Contributo in atti di convegno) (literal)
- Anno
- 2008-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1063/1.2905053 (literal)
- Alternative label
Farina D., Figini L., Platania P. and Sozzi C. (2008)
SPECE: A Code for Electron Cyclotron Emission in Tokamaks
in Int. Conf. Burning Plasma Diagnostics, Varenna, Italy, 24-28 September 2007
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Farina D., Figini L., Platania P. and Sozzi C. (literal)
- Pagina inizio
- Pagina fine
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
- http://proceedings.aip.org/resource/2/apcpcs/988/1/128_1 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#titoloVolume
- BURNING PLASMA DIAGNOSTICS: An International Conference (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#volumeInCollana
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#note
- AIP Conf. Proc., vol. 988, pp. 128-131 (2008) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- Istituto di Fisica del Plasma, CNR Milano. (literal)
- Titolo
- SPECE: A Code for Electron Cyclotron Emission in Tokamaks (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#isbn
- 978-0-7354-0507-3 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#curatoriVolume
- Giuseppe Gorini, Francesco P. Orsitto, Elio Sindoni, Marco Tardocchi (literal)
- Abstract
- The code SPECE has been developed for the analysis of electron cyclotron emission (ECE) in a general tokamak equilibrium. The code solves the radiation transport equation along the ray trajectories in a tokamak plasma, in which magnetic equilibrium and plasma profiles are given either analytically or numerically, for a Maxwellian plasma or a non thermal plasma characterized by a distribution function that is the sum of drifting Maxwellian distributions. Ray trajectories are computed making use of the cold dispersion relation, while the absorption and emission coefficients are obtained solving the relevant fully relativistic dispersion relation valid at high electron temperature. The actual antenna pattern is simulated by means of a multi-rays calculation, and the spatial resolution of the ECE measurements is computed by means of an algorithm that takes properly into account the emission along each ray of the beam. Wall effects are introduced in the code by means of a heuristic model. Results of ECE simulations in a standard ITER scenario are presented. (literal)
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