| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.20 | 87.31 | 12.82 | 44.40 | -4.73 | 31.38 | 5.41 | 205.09 | 0.2248 | 468.7 | 458.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.34 | 24.85 | 5.78 | 12.66 | -4.10 | 33.70 | 7.73 | 215.44 | 0.2323 | 1124.9 | 740.7 | |
| 1.17 | 5.76 | 0.59 | 2.92 | -4.14 | 32.07 | 6.10 | 209.24 | 0.2180 | 1004.2 | 750.5 | |
| 0.00 | 3.60 | 0.00 | 1.83 | -4.60 | 32.08 | 6.11 | 208.24 | 0.2250 | 922.0 | 760.2 | |
| 1.98 | 15.12 | 1.01 | 7.68 | -4.44 | 31.74 | 5.77 | 207.23 | 0.2200 | 1122.6 | 953.5 | |
| 0.00 | 1.89 | 0.00 | 0.96 | -4.96 | 31.38 | 5.40 | 204.73 | 0.2253 | 948.0 | 851.4 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -4.99 | 31.19 | 5.22 | 203.94 | 0.2244 | 767.0 | 671.8 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -2.58 | 30.97 | 5.00 | 208.10 | 0.1855 | 894.0 | 680.8 | |
| 4.59 | 9.27 | 2.33 | 4.71 | -4.77 | 30.86 | 4.88 | 202.93 | 0.2187 | 1122.3 | 754.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -5.95 | 30.86 | 4.89 | 201.03 | 0.2374 | 836.0 | 637.3 | |
| 0.00 | 1.98 | 0.00 | 1.01 | -5.33 | 30.80 | 4.83 | 201.74 | 0.2271 | 925.0 | 808.1 | |
| 2.97 | 7.11 | 1.51 | 3.61 | -5.37 | 29.15 | 3.18 | 194.65 | 0.2191 | -1082.8 | -834.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -3.92 | 29.08 | 3.11 | 196.22 | 0.1948 | -729.0 | -539.3 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -5.74 | 29.03 | 3.06 | 193.71 | 0.2248 | -876.0 | -729.4 | |
| 1.89 | 7.83 | 0.96 | 3.96 | -4.53 | 28.90 | 2.93 | 194.52 | 0.2042 | -1113.7 | -835.6 | |
| 0.00 | 2.34 | 0.00 | 1.24 | -13.34 | 28.90 | 2.93 | 188.21 | 0.3496 | -1.0 | -7.6 | |
| 1.26 | -14.00 | 0.64 | -14.00 | -4.35 | 28.78 | 2.81 | 194.16 | 0.2005 | -946.1 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -3.50 | 25.65 | -0.33 | 178.19 | 0.1801 | 836.0 | 632.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -5.39 | 23.30 | -2.68 | 167.61 | 0.2175 | -890.0 | -704.6 | |
| 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. | |