group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
50.11 | 248.24 | 26.90 | 133.21 | 14.80 | 255.32 | 6.88 | 342.41 | 0.3848 | -990.9 | -357.6 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 2.45 | 0.00 | 1.31 | 12.60 | 258.92 | 10.47 | 331.59 | 0.3745 | -725.0 | -599.4 | |
0.00 | 1.14 | 0.00 | 0.61 | 13.61 | 256.90 | 8.46 | 337.51 | 0.3753 | -780.0 | -679.8 | |
30.75 | 226.17 | 16.51 | 121.49 | 14.88 | 255.67 | 7.23 | 341.64 | 0.3875 | -1134.0 | -337.1 | |
0.44 | -3.00 | 0.23 | -3.00 | 14.61 | 255.16 | 6.72 | 342.64 | 0.3810 | -1076.2 | 999999 | |
0.00 | 2.37 | 0.00 | 1.26 | 14.04 | 255.11 | 6.67 | 342.28 | 0.3718 | -677.0 | -556.1 | |
18.92 | -3.00 | 10.16 | -3.00 | 15.09 | 254.96 | 6.52 | 343.50 | 0.3874 | -1131.1 | 999999 | |
0.00 | 4.03 | 0.00 | 2.12 | 12.25 | 254.81 | 6.37 | 341.46 | 0.3426 | -826.0 | -756.0 | |
0.00 | 1.58 | 0.00 | 0.83 | 12.91 | 254.43 | 5.99 | 343.09 | 0.3510 | -872.0 | -704.6 | |
0.00 | 2.10 | 0.00 | 1.12 | 14.57 | 254.01 | 5.57 | 345.44 | 0.3752 | -898.0 | -690.0 | |
0.00 | 1.31 | 0.00 | 0.69 | 11.76 | 253.60 | 5.16 | 344.41 | 0.3291 | -910.0 | -775.4 | |
0.00 | 2.01 | 0.00 | 1.05 | 10.50 | 253.52 | 5.08 | 343.55 | 0.3086 | -846.0 | -581.3 | |
0.00 | 1.93 | 0.00 | 1.02 | 12.68 | 253.53 | 5.09 | 345.34 | 0.3433 | -758.0 | -641.3 | |
0.00 | 1.14 | 0.00 | 0.63 | 19.06 | 252.24 | 3.80 | 351.78 | 0.4401 | -610.0 | -428.5 | |
0.00 | 2.01 | 0.00 | 1.08 | 15.00 | 251.54 | 3.09 | 351.96 | 0.3742 | 895.0 | 745.4 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |