2011
DOI: 10.1063/1.3557825
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Relationship between neutron yield rate of tokamak plasmas and spectrometer measured flux for different sight lines

Abstract: A parametric relationship between total neutron yield rate and collimated fluxes related to the brightness (B) of plasma chords (λ) is developed for different emissivity distributions of tokamak plasmas. Specifically, the brightness was expressed as a function of chord coordinates of radial position using a simple model for the emissivity profiles of width parameter w. The functional brightness dependence B(λ,w) was calculated to examine the relationship between measured flux and deduced yield rate, and its pl… Show more

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Cited by 4 publications
(9 citation statements)
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“…The LOS effect on the neutron spectrum was evaluated by calculating the collimated brightness B(p) along a given chord λ(p) [24]. The collimated brightness B(p), which is proportional to the neutron flux impinging on the detector, is defined as…”
Section: Monte Carlo Calculation Resultsmentioning
confidence: 99%
“…The LOS effect on the neutron spectrum was evaluated by calculating the collimated brightness B(p) along a given chord λ(p) [24]. The collimated brightness B(p), which is proportional to the neutron flux impinging on the detector, is defined as…”
Section: Monte Carlo Calculation Resultsmentioning
confidence: 99%
“…In this context it is interesting to note that, with a NES diagnostic, one could also provide support in the determination of the absolute value of the neutron yield rate of the EAST plasmas, i.e. the calibration of neutron flux monitors [25].…”
Section: Simulated Nes Results and Discussionmentioning
confidence: 99%
“…In the following, we shall further adopt the notation of [25] and use y γ (s) to denote the local gamma-ray emissivity. This will be a function of a radial coordinate s in the poloidal plane and gives the number of gamma-rays/second/cm 3 born at each plasma position.…”
Section: Generalized Abel Inversion Methods For the Jet Gamma-ray Cameramentioning
confidence: 99%
“…where y 0 is the peak emissivity, typically occurring on the magnetic axis, and ν is the peaking factor. The latter is related to the half width w of the profile by [25]…”
Section: Inversion Of Parabolic Emissivity Profilesmentioning
confidence: 99%