Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Plasma edge

As with pure SmS under pressure (37), the above metallized ICF conditions yield 9c) a free-carrier plasma edge which, though reaching well into the visible, is found to be restrained by 1/2 eV, compared with simple J metals like YS 9c) or LaS (or/" d GdS 12a) also). In line with this observation, and even more striking, is that the nett d.c. resistivity is actually increased upon going from B to M. Clearly, after the Sm/ d sites finally do become joined in d-band activities, the continual annihilation and creation of carriers at the Sm sites constitutes a strong scattering... [Pg.76]

Plasma impurities may also have a beneficial effect by cooling the plasma edge in the vicinity of the first wall. But this is partially offset by the fact that the sputtering yields due to impurities are higher as compared with that of hydrogen. Consequently, a relatively small concentration of impurities can significantly increase the wall erosion and plasma contamination. [Pg.60]

Any redeposition of sputtered wall atoms between burn cycles will make blistering more probable and more rapid. It appears that stainless steel first walls will suffer exfoliation for plasma edge temperatures below 100 eV, at all first-wall temperatures. Blistering can be expected to occur within 103 h of operation of a fusion power reactor. [Pg.81]

High electrical conductivity of organic conductors manifests itself in the IR spectra as anisotropic metal-like reflectivity associated with intermo-lecular charge transfer. Although an electron gas giving the plasma edge... [Pg.243]

TTF type. The optical anisotropy of such two-dimensional conductors and their electron parameters may also be deduced from reflectance studies. As an example, from the (TMTSF)2X family we present the polarized reflectance of (TMTSF)2PF6 at three temperatures (Fig. 7). It is evident that optical anisotropy decreases at low temperature, and a reasonably well-defined plasma edge appears in the b direction at 25 K. The transverse reflectance edge appears at the frequency about 10 times lower than that of the stacking axis edge (tb< = 22 meV, about 10 times smaller than ta) [46]. Drude parameters for typical (TMTSF)2X salt are eq = 3.5, 1500 cm-1 < cop < 2000 cm-1, 250 cm-1 < y < 500 cm-1, and tb = 0.02 eV. [Pg.245]

Despite these limitations computer simulations have become a key method in dealing with the various critical issues related to plasma edge phenomena on the path towards economical fusion power reactors, by quantifying at least the known parts of edge science, in a most detailed and complete way possible today. [Pg.32]

Using these standard notations one obtains the ten equations listed now. The terms Sn[fa] in these equations due to atomic and molecular interactions with neutral particle species n will be detailed below. For simplicity here the fluctuation term will not be considered. It is common (bad) practise in plasma edge modeling to account for its effect only in an ad-hoc manner (see below) after the fluid equations have first been derived without it. A comprehensive discussion, and proper derivation with this term included from the beginning, for plasma edge models, is given in [4]. [Pg.39]

A. Pospieszczyk High Temperature Plasma Edge Diagnostic. In this volume... [Pg.60]


See other pages where Plasma edge is mentioned: [Pg.391]    [Pg.402]    [Pg.423]    [Pg.92]    [Pg.287]    [Pg.310]    [Pg.412]    [Pg.423]    [Pg.444]    [Pg.261]    [Pg.27]    [Pg.361]    [Pg.148]    [Pg.368]    [Pg.54]    [Pg.60]    [Pg.63]    [Pg.94]    [Pg.391]    [Pg.402]    [Pg.423]    [Pg.393]    [Pg.244]    [Pg.245]    [Pg.454]    [Pg.458]    [Pg.5]    [Pg.6]    [Pg.30]    [Pg.30]    [Pg.31]    [Pg.32]    [Pg.34]    [Pg.34]    [Pg.38]    [Pg.52]    [Pg.59]    [Pg.63]    [Pg.99]    [Pg.99]    [Pg.100]   
See also in sourсe #XX -- [ Pg.335 ]

See also in sourсe #XX -- [ Pg.134 ]

See also in sourсe #XX -- [ Pg.308 , Pg.309 , Pg.313 , Pg.318 , Pg.320 , Pg.326 , Pg.368 ]




SEARCH



© 2024 chempedia.info