1994
DOI: 10.13182/fst94-a40229
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Development of an ITER Pellet Fueling System in Russia

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Cited by 7 publications
(6 citation statements)
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“…The scaling was obtained for a uniform distribution of the heating power inside the cloud, a monoenergy electron heat flux and a sonic-transonic regime in the molecular hydrogen flow. Our recent analysis of the cloud gas dynamics with Maxwellian electrons [27] has confirmed this scaling. Only the numerical factor is to be reduced by 0.66.…”
Section: (46supporting
confidence: 62%
“…The scaling was obtained for a uniform distribution of the heating power inside the cloud, a monoenergy electron heat flux and a sonic-transonic regime in the molecular hydrogen flow. Our recent analysis of the cloud gas dynamics with Maxwellian electrons [27] has confirmed this scaling. Only the numerical factor is to be reduced by 0.66.…”
Section: (46supporting
confidence: 62%
“…The main idea is that the effective area intercepting the electron heat flux, i.e., the projected area of the pellet normal to the B field is the main factor that determines the ablation rate. 10,11,14 For a spherical pellet, the projected area is half the surface area of the pellet, hence the factor of 2 reduction. A different result, factor of ϳ0.68 reduction, was found in MacAulays's simulation, 11 although it should be mentioned that the simulation in 1D ͑isotropic heating͒ was not possible.…”
Section: Ablation With Anisotropic Heatingmentioning
confidence: 99%
“…A further approximation, especially for energetic electrons with EϾ300-500 eV, is to neglect the weak energy dependence in the Coulomb logarithm. The solution of the kinetic equation for the distribution function of electrons traveling in the right ϩz ͑left Ϫz) directions that have penetrated a line-integrated density ϩ ( Ϫ ) is given by 10,29,30 f Ϯ ͑ E,, Ϯ ͒ϭ f max ͑ EЈ͒ ͩ When the ablation cloud is fully ionized and has no bulk motion, the heating rate given by Eq. ͑1c͒ and the definition of e in Eq.…”
Section: Appendix: Derivation Of Semianalytic Kinetic Heat Flux Exprementioning
confidence: 99%
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“…This is because the net particle flux is relatively small due to backscatter in the high-Z case. The diffusion equation, equation (14), indicates that the incident electron flux scales as n ∞ v th /Z 1/2 , which is a factor Z 1/2 lower as compared to the case when there is no scattering. This particle flux is used to calculate the sheath potential in the appendix, and we show that the sheath potential required to maintain ambipolarity scales as Z −1/3 .…”
Section: Physics Modelmentioning
confidence: 99%