Results 141 to 150 of about 464 (186)

Stellarators and Optimised Stellarators

Fusion Technology, 1998
The properties of a classical stellarator will be described and the need to optimise stellarators will be motivated. The principles of optimisation will be presented. W7-AS, a partly optimised modular stellarator, will be briefly introduced and some results with relevance to its optimised properties will be summarised.
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The Stellarator Concept

IEEE Transactions on Plasma Science, 1958
The basic concepts of the controlled thermonuclear program at Project Matterhorn, Princeton University are discussed. In particular, the theory of confinement of a fully ionized gas in the magnetic configuration of the stellarator is given, the theories of heating are outlined, and the bearing of observational results on these theories is described.
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Stellar Inversions

Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Transport in stellarators

Plasma Physics and Controlled Fusion, 1993
The local electron and ion heat transport as well as the particle and impurity transport properties in stellarators are reviewed. In this context, neoclassical theory is used as a guideline for the comparison of the experimental results of the quite different confinement concepts.
Maassberg, H., Brakel, R., Burhenn, R., Gasparino, U., Grigull, P., Kick, M., Kuhner, G., Ringler, H., Sardei, F., Stroth, U., Weller, A.   +10 more
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Stellar Convection

Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Demarque, Pierre, Robinson, Francis J.
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Stellar Populations, Stellar Evolution, and Stellar Atmospheres

2021
J. J. Eldridge, E. R. Stanway
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Stellar Evolution and Stellar Structures

1995
It is often thought that very little was known about the stars in the nineteenth century because most astronomy books of the time tended to concentrate on the planets. This was far from the truth, however, although nineteenth century knowledge of the stars was purely observational, with no understanding of their internal processes. In fact, at the time
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Stellar Radii

Symposium - International Astronomical Union, 1997
Observing a stellar radius basically means observing a center-to-limb intensity variation. The significance and properties of center-to-limb variations, common approximations, the correlation with optical-depth radii in extended-photophere stars, and direct measurements of angular (interferometry, lunar occultation) and absolute diameters (binary ...
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Stellar chromospheres.

Science (New York, N.Y.), 1966
Besides being of intrinsic interest, these outer stellar envelopes provide very useful astrophysical tools.
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Wendelstein stellarators

Nuclear Fusion, 1985
Grieger, G., Renner, H., Wobig, H.
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