| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 518 | 49 | 266 | -10.44 | 276.57 | 0.01 | 182.14 | 0.2635 | -729.4 | -331.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 305 | 23 | 155 | -9.38 | 279.93 | 3.37 | 193.97 | 0.2412 | -1945.1 | -717.2 | |
| 0 | 4 | 0 | 2 | -10.01 | 278.76 | 2.20 | 188.82 | 0.2478 | -838.0 | -642.1 | |
| 16 | 40 | 8 | 21 | -9.77 | 277.98 | 1.42 | 185.81 | 0.2420 | -1323.9 | -639.9 | |
| 0 | 10 | 0 | 5 | -8.86 | 277.04 | 0.48 | 182.11 | 0.2254 | -969.0 | -705.3 | |
| 0 | 4 | 0 | 2 | -8.86 | 276.57 | 0.01 | 180.05 | 0.2253 | -489.0 | -427.6 | |
| 0 | 6 | 0 | 3 | -11.36 | 276.45 | -0.11 | 179.61 | 0.2678 | 685.0 | 557.6 | |
| 0 | 7 | 0 | 3 | -10.32 | 275.99 | -0.57 | 177.73 | 0.2504 | 476.0 | 399.2 | |
| 2 | 9 | 1 | 5 | -12.99 | 270.48 | -6.08 | 160.62 | 0.3125 | -506.0 | -326.2 | |
| 5 | 13 | 2 | 7 | -13.88 | 270.30 | -6.26 | 161.04 | 0.3274 | -1107.3 | -833.1 | |
| 0 | 11 | 0 | 6 | -13.19 | 270.04 | -6.52 | 159.56 | 0.3182 | 669.0 | 546.4 | |
| 0 | 9 | 0 | 5 | -16.37 | 269.74 | -6.82 | 161.92 | 0.3690 | -988.0 | -801.6 | |
| 13 | 56 | 7 | 29 | -11.63 | 269.48 | -7.08 | 155.97 | 0.2976 | 1608.0 | 912.6 | |
| 0 | 6 | 0 | 3 | -13.44 | 269.35 | -7.21 | 157.92 | 0.3261 | 979.0 | 765.2 | |
| 5 | -12 | 3 | -12 | -11.79 | 269.12 | -7.44 | 155.12 | 0.3026 | 1200.7 | 999999 | |
| 0 | 7 | 0 | 3 | -13.33 | 268.32 | -8.24 | 154.98 | 0.3313 | 677.0 | 597.5 | |
| 9 | 31 | 5 | 17 | -13.46 | 267.67 | -8.89 | 153.46 | 0.3378 | 1219.3 | 994.5 | |
| 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. | |