| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.30 | 154.44 | 48.16 | 97.47 | 8.98 | 99.87 | -36.37 | 70.79 | 0.6225 | 20.1 | 145.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.97 | 11.64 | 4.27 | 7.13 | 9.06 | 102.30 | -33.94 | 69.44 | 0.5911 | -1048.1 | -717.4 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 9.31 | 102.13 | -34.11 | 69.13 | 0.5945 | -751.0 | -721.4 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 9.58 | 102.03 | -34.21 | 68.75 | 0.5971 | -793.0 | -648.8 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 9.80 | 101.93 | -34.31 | 68.47 | 0.5994 | -563.0 | -490.3 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 9.23 | 101.89 | -34.35 | 69.40 | 0.5973 | -627.0 | -496.8 | |
| 0.51 | 3.31 | 0.31 | 2.05 | 9.44 | 101.76 | -34.49 | 69.13 | 0.6001 | -671.7 | -502.5 | |
| 0.00 | 1.19 | 0.00 | 0.74 | 9.87 | 101.63 | -34.61 | 68.52 | 0.6036 | -624.0 | -487.0 | |
| 1.27 | 2.55 | 0.79 | 1.58 | 9.55 | 101.27 | -34.97 | 69.21 | 0.6069 | -618.6 | -362.2 | |
| 0.00 | 1.78 | 0.00 | 1.11 | 9.74 | 101.14 | -35.11 | 68.99 | 0.6095 | 111.0 | -185.0 | |
| 23.28 | 32.54 | 14.45 | 20.20 | 8.06 | 100.92 | -35.32 | 71.74 | 0.6051 | -880.1 | -326.8 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 9.52 | 100.54 | -35.70 | 69.64 | 0.6162 | 658.0 | 468.1 | |
| 0.00 | 4.08 | 0.00 | 2.56 | 8.09 | 100.11 | -36.14 | 72.07 | 0.6159 | 45.0 | -135.8 | |
| 1.19 | 54.71 | 0.76 | 34.98 | 9.50 | 99.46 | -36.78 | 70.20 | 0.6299 | 812.4 | 467.8 | |
| 0.00 | 4.08 | 0.00 | 2.58 | 8.35 | 99.56 | -36.68 | 71.92 | 0.6241 | 273.0 | 38.9 | |
| 16.91 | 30.33 | 10.83 | 19.40 | 10.00 | 99.06 | -37.18 | 69.65 | 0.6371 | 802.4 | 776.2 | |
| 0.00 | 1.70 | 0.00 | 1.08 | 8.37 | 99.07 | -37.17 | 72.11 | 0.6305 | -353.0 | -235.9 | |
| 26.17 | -13.00 | 16.75 | -13.00 | 8.95 | 98.82 | -37.43 | 71.34 | 0.6360 | 808.4 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 5.62 | 98.13 | -38.12 | 76.70 | 0.6335 | -456.0 | -416.3 | |
| 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. | |