Stationary and axisymmetric magnetized equilibria of stars and winds

Shin Yoshida, Kotaro Fujisawa, Yoshiharu Eriguchi, Shijun Yoshida, Rohta Takahashi

研究成果: Conference contribution

抜粋

We present a new formulation to compute numerically stationary and axisymmetric equilibria of magnetized and self-gravitating astrophysical fluids. Under the assumption of ideal MHD, the stream function for the flow can be chosen as a basic variable with which the Euler-Maxwell equations are cast into a set of basic equations, i.e. a generalized Bernoulli equation and a Grad-Shafranov-like equation by employing various integral conditions. A novel feature of this formulation is that systems with stars, disks and winds are treated in a simple unified picture and the magnetic field structures can contain both poloidal and toroidal components.

元の言語English
ホスト出版物のタイトルProceedings of the International Astronomical Union
ページ437-440
ページ数4
6
エディションS274
DOI
出版物ステータスPublished - 2010 9
外部発表Yes

出版物シリーズ

名前Proceedings of the International Astronomical Union
番号S274
6
ISSN(印刷物)17439213
ISSN(電子版)17439221

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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  • これを引用

    Yoshida, S., Fujisawa, K., Eriguchi, Y., Yoshida, S., & Takahashi, R. (2010). Stationary and axisymmetric magnetized equilibria of stars and winds. : Proceedings of the International Astronomical Union (S274 版, 巻 6, pp. 437-440). (Proceedings of the International Astronomical Union; 巻数 6, 番号 S274). https://doi.org/10.1017/S1743921311007435