Table 2.
Plasma flow velocities reconstructed in NOAA AR open loop 3D points.
| vLOS1 | vLOS2 | vep | β | V3D | |
|---|---|---|---|---|---|
| (km s−1) | (km s−1) | (km s−1) | (degrees) | (km s−1) | |
| Open loop | |||||
| Point 4 | −13.61 km s−1 | −16.71 km s−1 | −16.73 km s−1 | 28.86° | −19.11 km s−1 |
| Point 5 | −4.54 km s−1 | −5.67 km s−1 | −5.67 km s−1 | 28.54° | −6.45 km s−1 |
| Open loop | |||||
| Point 6 | −3.37 km s−1 | −5.27 km s−1 | −5.45 km s−1 | 36.29° | −6.76 km s−1 |
| Point 7 | −2.03 km s−1 | −3.17 km s−1 | −3.29 km s−1 | 36.32° | −4.07 km s−1 |
Notes. Numerical values of the fully reconstructed velocity vectors V3D, which characterise outflows along open loops shown by black arrows in Fig. 9. β is the angle between the velocity vector vep measured in the epipolar plane and the loop. V3D can be reconstructed by deprojecting vep onto the coronal loop. The calculations were carried out for each of the points 4, 5, 6, and 7, which lie on open loops. The minus sign is implied to indicate outflows.
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