| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.18 | 0.00 | 14.25 | 4.29 | 255.74 | 6.01 | 279.22 | 0.1801 | 371.7 | 377.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.73 | 5.31 | 272.42 | 22.69 | 282.86 | 0.3956 | -764.0 | -701.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 3.17 | 271.95 | 22.22 | 277.61 | 0.3826 | -758.0 | -601.4 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 0.26 | 268.05 | 18.32 | 269.92 | 0.3157 | -945.0 | -689.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -0.29 | 268.02 | 18.29 | 268.18 | 0.3153 | -871.0 | -684.9 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 4.39 | 262.09 | 12.36 | 288.48 | 0.2261 | 753.0 | 565.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 4.57 | 261.78 | 12.06 | 289.70 | 0.2221 | 718.0 | 552.7 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 6.25 | 260.23 | 10.50 | 299.81 | 0.2097 | 766.0 | 628.0 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 6.22 | 260.01 | 10.28 | 300.20 | 0.2062 | 944.0 | 684.1 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 5.81 | 253.19 | 3.46 | 327.96 | 0.1137 | 908.0 | 555.0 | |
| 0.00 | 1.18 | 0.00 | 0.58 | 0.54 | 252.80 | 3.07 | 274.41 | 0.0540 | 893.0 | 657.3 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 9.52 | 252.73 | 3.00 | 342.13 | 0.1691 | 761.0 | 548.8 | |
| 0.00 | 3.17 | 0.00 | 1.59 | 7.98 | 252.41 | 2.68 | 340.90 | 0.1421 | 828.0 | 633.5 | |
| 0.00 | 4.26 | 0.00 | 2.12 | 5.32 | 250.37 | 0.64 | 352.71 | 0.0887 | 788.0 | 855.3 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 5.63 | 250.37 | 0.65 | 353.11 | 0.0940 | 766.0 | 645.1 | |
| 0.00 | 4.35 | 0.00 | 2.17 | 1.00 | 242.92 | -6.80 | 84.07 | 0.1196 | 788.0 | 698.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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 | |
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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. | |