Image Details

Choose export citation format:

Field-aligned and Magnetic Reconnection Flows in a Magnetohydrodynamic Simulation of Prominence-cavity System

  • Authors: Tie Liu, Yingna Su, Yang Guo, Jie Zhao, Haisheng Ji

Tie Liu et al 2023 The Astrophysical Journal 949 .

  • Provider: AAS Journals

Caption: Figure 7.

Two rings in the synthetic Doppler image. Panel (a) is similar to Figure 6(a), but with CMER = −87° and BANG = 9° for time = 13.88 hr. Panel (c) is the same as panel (a) but for time = 18.24 hr. The corresponding velocity changes along the line slices (thick solid green lines) from the beginning to the end are displayed in panels (b) and (d), respectively. We mark the two peaks generated by the field-aligned flows as ring1 and ring2.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse