Abstract
Magnetic surface breaking due to the finite pressure effect is analyzed for three dimensional magnetohydrodynamic equilibria of 1=2 Heliotron configuration. Characteristics of magnetic island formation are extensively surveyed. It is found that the well-hill criterion which has been predicted by the local analysis is not always applicable for all cases. (author).
Citation Formats
Hayashi, Takaya, Takei, Akira, and Sato, Tetsuya.
Magnetic surface breaking in 3D MHD equilibria of 1=2 Heliotron.
Japan: N. p.,
1992.
Web.
Hayashi, Takaya, Takei, Akira, & Sato, Tetsuya.
Magnetic surface breaking in 3D MHD equilibria of 1=2 Heliotron.
Japan.
Hayashi, Takaya, Takei, Akira, and Sato, Tetsuya.
1992.
"Magnetic surface breaking in 3D MHD equilibria of 1=2 Heliotron."
Japan.
@misc{etde_10111079,
title = {Magnetic surface breaking in 3D MHD equilibria of 1=2 Heliotron}
author = {Hayashi, Takaya, Takei, Akira, and Sato, Tetsuya}
abstractNote = {Magnetic surface breaking due to the finite pressure effect is analyzed for three dimensional magnetohydrodynamic equilibria of 1=2 Heliotron configuration. Characteristics of magnetic island formation are extensively surveyed. It is found that the well-hill criterion which has been predicted by the local analysis is not always applicable for all cases. (author).}
place = {Japan}
year = {1992}
month = {Jan}
}
title = {Magnetic surface breaking in 3D MHD equilibria of 1=2 Heliotron}
author = {Hayashi, Takaya, Takei, Akira, and Sato, Tetsuya}
abstractNote = {Magnetic surface breaking due to the finite pressure effect is analyzed for three dimensional magnetohydrodynamic equilibria of 1=2 Heliotron configuration. Characteristics of magnetic island formation are extensively surveyed. It is found that the well-hill criterion which has been predicted by the local analysis is not always applicable for all cases. (author).}
place = {Japan}
year = {1992}
month = {Jan}
}