All Tables

• Table 1: Effective heights of coronal bright points calculated for various latitude bins using Eqs. (11) and (12) for the interactive method. The results for all data and for the subsample of point-like structures (PLS) are presented.
• Table 2: Differential rotation parameters A, B, and C from Eq. (15) for the interactive method, without the height correction. The sidereal parameters and their standard errors (M) are expressed in deg/day for three cases (see remarks). Both solar hemispheres are treated together and the number of tracers n=1179 (after the velocity filter was applied).
• Table 3: As Table 2 with the height correction (interactive method). n=1182.
• Table 4: As Table 2 for the automatic method (without the height correction). n=1500.
• Table 5: As Table 3 for the automatic method (with the height correction). n=1495.
• Table 6: A comparison of differential rotation parameters A, B, and C from Eq. (15) for coronal bright points (Tables 2-5) with other results. R - remark.