1986
DOI: 10.1088/0741-3335/28/9a/008
|View full text |Cite
|
Sign up to set email alerts
|

A review of Alfven wave heating

Abstract: This paper r e v i w s the experimental status and recevt advances i n AlfvCn Wave Heating (AWH). We discuss the underlying physics of Alfven Wave Heating, as seen by the experiments. The use of AlfvCn Waves for plasna diagnosis is discussed. The results of plasna heating on TCA are s m a r i z e d . Apparent changes i n the current profile are inferred, caused by changes i n the evolving AlfvCn wave spectrun excited. The implications for AWH on larger devices are mentioned. KFrwoRDsAlfven Wave Heating; Tokama… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
9
0

Year Published

1988
1988
2010
2010

Publication Types

Select...
8

Relationship

1
7

Authors

Journals

citations
Cited by 22 publications
(10 citation statements)
references
References 17 publications
1
9
0
Order By: Relevance
“…The resulting dispersion behavior is directly related to heat and energy transport in magnetized plasmas [3]. This is observed in laboratory [4][5][6][7] and fusion devices [8,9] as well as in space plasmas, e.g., the solar atmosphere [10] or during the interaction between the solar wind with the cusp regions of the terrestrial magnetoshere [11]. AWs are responsible for heating of the solar corona [12] and acceleration of the solar wind [13,14] by transferring energy from the sun's photosphere to the chromosphere in so-called flux tubes [15].…”
Section: Introduction and Basicsmentioning
confidence: 86%
“…The resulting dispersion behavior is directly related to heat and energy transport in magnetized plasmas [3]. This is observed in laboratory [4][5][6][7] and fusion devices [8,9] as well as in space plasmas, e.g., the solar atmosphere [10] or during the interaction between the solar wind with the cusp regions of the terrestrial magnetoshere [11]. AWs are responsible for heating of the solar corona [12] and acceleration of the solar wind [13,14] by transferring energy from the sun's photosphere to the chromosphere in so-called flux tubes [15].…”
Section: Introduction and Basicsmentioning
confidence: 86%
“…The additional heating was provided by Alfven Waves launched by 8 phase-coherent antennae. The TCA Tokamak has been described in detail by CHEETHAM et al (1981) and the Alfven Wave excitation and heating experiments by COLLINS et al BESSON et al (1986). The r.f.…”
Section: E X P E R I M E N T a N D M E T H O Dmentioning
confidence: 99%
“…For the specific case of the ion-ion hybrid, and using Eq. (27) for simplicity, we shall also be able to show how to determine which sign to use in Eq. (43) of ref.…”
Section: Fig 2 Variation Of the Fw's Wavevector(squared) Overmentioning
confidence: 99%
“…From the experimental point of view the most extensive experiments and analysis of Alfvén wave heating have been performed on the TCA tokamak 27 (R 0 =0.6m). Although antenna coupling and general wave behaviour appeared to be in agreement with the theory, generally speaking little plasma heating was observed while the main effect of the RF was a large density increase, sometimes interpreted as an increase in the particle confinement time.…”
Section: Alfven Wave Heatingmentioning
confidence: 99%