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Table B.2.

Host granule properties

ID Type[1] < A> HG [ 2 ] $ _{\mathrm{HG}}^{[2]} $ HG Cov[3] v(z)low[4] v(z)middle[4] v(z)high[4] σv(z)low[5] σv(z)middle[5] σv(z)high[5]
[Mm2] [%] [km s−1] [km s−1] [km s−1] [km s−1] [km s−1] [km s−1]
100 GL 1.5 36 -0.25 -0.15 -0.09 0.6 0.44 0.32
801 EG 1.4 39 -0.72 -0.54 -0.39 0.35 0.32 0.28
352 NG 1.1 58 -0.28 -0.14 -0.08 0.41 0.33 0.29
577 CG[6]
296 EG 1.1 31 -0.92 -0.75 -0.69 0.42 0.31 0.24
1 EG 1.9 71 -0.48 -0.26 -0.06 0.48 0.41 0.39
239 GL 1.5 28 -0.6 -0.46 -0.36 0.58 0.45 0.37
799 EG 1.1 43 -0.76 -0.52 -0.39 0.28 0.25 0.2
29 EG 1.6 20 -0.11 -0.06 0 0.48 0.36 0.3
48 EG 1.2 39 -0.32 -0.2 -0.11 0.34 0.27 0.23
432 GL 1.5 20 -0.43 -0.2 -0.06 0.39 0.35 0.32
641 GL 1.6 22 -0.83 -0.65 -0.47 0.44 0.42 0.39
345 EG 1.8 24 -0.91 -0.75 -0.66 0.42 0.32 0.27
347 GL 1.2 55 -0.57 -0.38 -0.24 0.29 0.27 0.26
440 GL 2.3 20 -0.81 -0.66 -0.57 0.51 0.51 0.48
260 CG
572 NG 0.9 14 -0.54 -0.35 -0.26 0.37 0.29 0.26
180 EG 3 14 -0.58 -0.37 -0.26 0.35 0.31 0.29
184 CG
187 EG 1.4 18 -0.62 -0.4 -0.33 0.32 0.25 0.21
458 NG 0.4 48 -0.09 -0.04 -0.04 0.48 0.37 0.35
523 NG 1.1 34 -0.63 -0.45 -0.36 0.57 0.48 0.4
297 NG 1.2 30 -0.51 -0.28 -0.18 1.22 0.51 0.42
460 NG 1.1 38 -0.01 0.03 0.05 0.65 0.48 0.4
347 GL 1.4 24 -0.01 0.08 0.14 0.58 0.54 0.47
645 EG 1.1 67 -0.41 -0.3 -0.24 0.28 0.25 0.23
29372 GL 2.1 11 -0.18 -0.02 0.07 0.88 0.48 0.47
32927 NG 0.6 47 -0.48 -0.3 -0.16 0.27 0.28 0.24
53961 GL 1.1 18 -0.48 -0.36 -0.18 0.34 0.33 0.26
58570 EG 1.8 21 0.11 0.36 0.46 0.95 0.45 0.44
91772 EG 1.8 39 -0.31 -0.2 -0.1 0.54 0.45 0.44
94010 NG 0.4 41 -0.45 -0.31 -0.19 0.26 0.28 0.22
12232 NG 0.9 15 -0.35 -0.32 -0.31 0.37 0.39 0.41
16683 EG 5 8 -0.13 -0.15 -0.16 0.64 0.35 0.34
17058 EG 1.4 42 -0.89 -0.92 -0.89 0.56 0.54 0.55
22153 NG 0.5 35 -0.97 -0.37 -0.32 1.33 0.39 0.36
39266 GL 3.7 37 -0.13 -0.07 -0.06 0.65 0.41 0.4
58352 NG 1 61 -0.15 -0.18 -0.15 0.51 0.48 0.47
58366 NG 0.3 28 -0.04 0 0.02 0.31 0.27 0.25
60914 CG
112354 EG 1 24 -0.49 -0.54 -0.56 0.32 0.32 0.33
125941 GL 1.3 13 -0.23 -0.18 -0.15 0.76 0.44 0.45

Notes. [1] Type of granulation: EG - Exploding granules, NG - Nascent granules, GL - Granular lanes, CG - Complex granulation.[2] Mean area of the host granule.[3] Percent coverage of the magnetic flux sheet over the host granule.[4] Spatial average of the bisector velocities measured at low, middle and high heights in the photosphere.[5] Standard deviation of the bisector velocities measured at low, middle and high heights in the photosphere.[6] We excluded CG from the statistics on the host granule coverage and the plasma dynamics of host granules.

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