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Transfer processes in stellarators at the regime of frequent particle collisions; Protsessy perenosa v stellaratorakh v rezhime chastykh stolknovenij chastits

Abstract

Method of studying particle and heat fluxes in stellarators in the regime of frequent particle collisions and allowing for real geometry of their magnetic field is considered. 10 refs.; 2 figs.; 1 tab.
Authors:
Publication Date:
Dec 31, 1990
Product Type:
Technical Report
Report Number:
KFTI-90-8
Reference Number:
SCA: 700330; PA: AIX-24:004187; SN: 93000914128
Resource Relation:
Other Information: PBD: 1990
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; TORSATRON STELLARATORS; DIFFUSION; HEAT TRANSFER; COLLISIONAL PLASMA; ELECTRIC CURRENTS; IMPURITIES; MAGNETIC FIELDS; MAGNETIC SURFACES; NUMERICAL SOLUTION; SPATIAL DISTRIBUTION; 700330; PLASMA KINETICS, TRANSPORT, AND IMPURITIES
OSTI ID:
10109261
Research Organizations:
AN Ukrainskoj SSR, Kharkov (Ukraine). Fiziko-Tekhnicheskij Inst.
Country of Origin:
Ukraine
Language:
Russian
Other Identifying Numbers:
Other: ON: DE93610253; TRN: UA9200566004187
Availability:
OSTI; NTIS (US Sales Only); INIS
Submitting Site:
INIS
Size:
[16] p.
Announcement Date:
Jun 30, 2005

Citation Formats

Nemov, V V. Transfer processes in stellarators at the regime of frequent particle collisions; Protsessy perenosa v stellaratorakh v rezhime chastykh stolknovenij chastits. Ukraine: N. p., 1990. Web.
Nemov, V V. Transfer processes in stellarators at the regime of frequent particle collisions; Protsessy perenosa v stellaratorakh v rezhime chastykh stolknovenij chastits. Ukraine.
Nemov, V V. 1990. "Transfer processes in stellarators at the regime of frequent particle collisions; Protsessy perenosa v stellaratorakh v rezhime chastykh stolknovenij chastits." Ukraine.
@misc{etde_10109261,
title = {Transfer processes in stellarators at the regime of frequent particle collisions; Protsessy perenosa v stellaratorakh v rezhime chastykh stolknovenij chastits}
author = {Nemov, V V}
abstractNote = {Method of studying particle and heat fluxes in stellarators in the regime of frequent particle collisions and allowing for real geometry of their magnetic field is considered. 10 refs.; 2 figs.; 1 tab.}
place = {Ukraine}
year = {1990}
month = {Dec}
}