Image Details

Choose export citation format:

Asymmetric Transport of the Earth’s Polar Outflows by the Interplanetary Magnetic Field

  • Authors: Juan Wang, Can Huang, Yasong S. Ge, Aimin Du, Xueshang Feng, and Kun Li

2019 The Astrophysical Journal Letters 881 L34.

  • Provider: AAS Journals

Caption: Figure 3.

(a) Overview of the north–south asymmetric polar outflows during a typical southward IMF condition, under the influences of a Bx component. The gray lines are the magnetic field lines, the white arrows denote the flow vectors, and the red line denotes the specified streamline. The background colors represent the thermal pressure in the noon–midnight meridian plane. (b) The forces acting on the polar outflows along the specified streamline. The orange, green, and red lines denote the thermal pressure gradient, Ampère, and total forces along the streamline, respectively. The blue line represents the velocity.

Other Images in This Article
Copyright and Terms & Conditions