Results 141 to 150 of about 249 (184)
Some of the next articles are maybe not open access.
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. +10 more
openaire +3 more sources
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. +10 more
openaire +3 more sources
Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Demarque, Pierre, Robinson, Francis J.
openaire +2 more sources
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Demarque, Pierre, Robinson, Francis J.
openaire +2 more sources
Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire +1 more source
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire +1 more source
Stellar Populations, Stellar Evolution, and Stellar Atmospheres
2021J. J. Eldridge, E. R. Stanway
openaire +1 more source
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 ...
openaire +1 more source
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 ...
openaire +1 more source
Stellar Evolution and Stellar Structures
1995It 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
openaire +1 more source
Science (New York, N.Y.), 1966
Besides being of intrinsic interest, these outer stellar envelopes provide very useful astrophysical tools.
openaire +3 more sources
Besides being of intrinsic interest, these outer stellar envelopes provide very useful astrophysical tools.
openaire +3 more sources
Poor confinement in stellarators at high energy
Physics of Plasmas, 2022Stéphane Éthier +2 more
exaly