A magnetohydrodynamic simulation of the single-fluid 2-D structure of the solar wind

Author： Jin-Tao X. Jing-Fang W. Xin Q. Xiao-Hua D.

Publisher： Elsevier

ISSN： 0275-1062

Source： Chinese Astronomy and Astrophysics, Vol.27, Iss.3, 2003-07, pp. : 308-314

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

An axisymmetric magnetohydrodynamic model for the interaction of the solar wind with the local interstellar medium

By Aleksashov D. Baranov V. Barsky E. Myasnikov A.

Astronomy Letters, Vol. 26, Iss. 11, 2000-11 ,pp. : 743-749

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Two-fluid 2.5D MHD Simulations of the Fast Solar Wind in Coronal Holes and the Relation to UVCS Observations

By Davila J.M. Ofman L.

Space Science Reviews, Vol. 87, Iss. 1, 1999-01 ,pp. : 165-168

Springer Publishing Company

Access to resources Recommend Favorite

Structure of the Solar Wind and Compositional Variations

By Bochsler P.

Space Science Reviews, Vol. 85, Iss. 1-2, 1998-01 ,pp. : 291-302

Springer Publishing Company

Access to resources Recommend Favorite

Semi-Empirical 2-D MHD Model of the Solar corona and Solar Wind: Energy Flow in the Corona

By Sittler E. Guhathakurta M. Skoug R.

Space Science Reviews, Vol. 97, Iss. 1-4, 2001-01 ,pp. : 39-44

Springer Publishing Company

Access to resources Recommend Favorite

A model of Charge Exchange of Interstellar Hydrogen on a Time-Dependent, 2D Solar Wind

By Bzowski M.

Space Science Reviews, Vol. 97, Iss. 1-4, 2001-01 ,pp. : 379-383

Springer Publishing Company

Access to resources Recommend Favorite