| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.71 | 26.98 | 0.86 | 13.71 | 8.34 | 195.75 | -6.05 | 28.10 | 0.2183 | 55.5 | -93.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.95 | 0.00 | 2.00 | 8.17 | 198.59 | -3.21 | 16.66 | 0.1942 | -1388.0 | -1007.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 6.97 | 198.47 | -3.33 | 19.28 | 0.1752 | -983.0 | -802.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.13 | 198.38 | -3.42 | 19.48 | 0.1782 | -888.0 | -694.5 | |
| 1.71 | 3.95 | 0.86 | 2.00 | 8.51 | 197.70 | -4.10 | 20.32 | 0.2047 | -1173.1 | -901.2 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 8.39 | 197.42 | -4.38 | 21.79 | 0.2044 | -1003.0 | -787.2 | |
| 0.00 | 1.89 | 0.00 | 0.96 | 8.46 | 196.68 | -5.12 | 24.90 | 0.2105 | -831.0 | -751.9 | |
| 0.00 | 2.34 | 0.00 | 1.19 | 8.83 | 195.72 | -6.08 | 28.04 | 0.2235 | -570.0 | -422.1 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 6.96 | 194.95 | -6.85 | 35.80 | 0.2033 | 847.0 | 665.6 | |
| 0.00 | 2.07 | 0.00 | 1.05 | 7.58 | 194.45 | -7.35 | 35.97 | 0.2169 | 993.0 | 757.8 | |
| 0.00 | 1.80 | 0.00 | 0.92 | 9.40 | 194.01 | -7.79 | 32.99 | 0.2466 | 948.0 | 723.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 8.57 | 193.29 | -8.51 | 37.37 | 0.2423 | 915.0 | 637.4 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 7.68 | 193.27 | -8.53 | 39.80 | 0.2306 | 1020.0 | 786.5 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 8.73 | 193.16 | -8.64 | 37.38 | 0.2457 | 976.0 | 800.0 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 8.48 | 193.13 | -8.67 | 38.09 | 0.2427 | 883.0 | 799.1 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 9.74 | 190.36 | -11.44 | 42.78 | 0.2892 | 914.0 | 727.8 | |
| 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. | |