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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.