Figure 6: EIS Doppler velocity map of the solar corona at 2 MK with magnetic field lines overlaid. | Nature Communications

Figure 6: EIS Doppler velocity map of the solar corona at 2 MK with magnetic field lines overlaid.

From: Full-Sun observations for identifying the source of the slow solar wind

Figure 6

Overlay of magnetic field lines from our PFSS calculation on the Fe XIII 202.044 Å Doppler velocity map in Fig. 4. This time, the green field lines are open and the orange field lines are closed. Again, only a small subset of the total number of field lines we computed are shown: 287 in this case. As with Fig. 5, the field lines are selected randomly and we have drawn relatively more open-field lines for emphasis.

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