| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 482 | 55 | 335 | 18.89 | 31.52 | -42.70 | 66.17 | 0.7030 | 229.2 | 32.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 18.02 | 41.08 | -33.15 | 63.26 | 0.5844 | 653.0 | 639.0 | |
| 0 | 6 | 0 | 4 | 18.19 | 38.66 | -35.56 | 64.28 | 0.6155 | 566.0 | 356.5 | |
| 6 | 158 | 4 | 105 | 19.63 | 34.90 | -39.32 | 63.89 | 0.6670 | 1452.8 | 541.9 | |
| 18 | -3 | 12 | -3 | 19.29 | 34.72 | -39.50 | 64.45 | 0.6677 | 1171.4 | 999999 | |
| -4 | -3 | -4 | -3 | 19.57 | 34.37 | -39.85 | 64.21 | 0.6729 | 999999 | 999999 | |
| 13 | 24 | 9 | 17 | 20.54 | 32.55 | -41.67 | 63.59 | 0.6974 | 902.8 | 543.1 | |
| 0 | 6 | 0 | 4 | 20.16 | 32.23 | -41.99 | 64.25 | 0.6996 | 3.0 | 184.2 | |
| 0 | 14 | 0 | 9 | 18.06 | 32.71 | -41.51 | 66.99 | 0.6869 | -712.0 | -535.6 | |
| 0 | 8 | 0 | 5 | 19.48 | 31.99 | -42.23 | 65.27 | 0.6999 | 516.0 | 352.8 | |
| 0 | 5 | 0 | 3 | 19.20 | 31.11 | -43.11 | 65.98 | 0.7089 | 270.0 | 157.6 | |
| 0 | 2 | 0 | 2 | 19.64 | 30.73 | -43.49 | 65.51 | 0.7146 | -23.0 | -17.1 | |
| 0 | 6 | 0 | 4 | 20.42 | 30.34 | -43.88 | 64.60 | 0.7214 | -201.0 | -163.5 | |
| 4 | 25 | 3 | 18 | 17.92 | 31.11 | -43.11 | 67.73 | 0.7049 | -884.5 | -737.5 | |
| 8 | 199 | 5 | 143 | 18.61 | 29.79 | -44.43 | 67.21 | 0.7219 | -1203.2 | -231.8 | |
| 15 | -14 | 11 | -14 | 18.19 | 29.69 | -44.53 | 67.81 | 0.7218 | -1060.5 | 999999 | |
| 4 | -14 | 3 | -14 | 18.76 | 29.45 | -44.78 | 67.12 | 0.7262 | -592.7 | 999999 | |
| 11 | -14 | 8 | -14 | 18.80 | 28.30 | -45.92 | 67.42 | 0.7389 | 915.0 | 999999 | |
| 0 | 3 | 0 | 2 | 17.94 | 28.47 | -45.75 | 68.51 | 0.7347 | -484.0 | -395.3 | |
| 0 | 8 | 0 | 6 | 17.92 | 28.00 | -46.22 | 68.66 | 0.7399 | -519.0 | -416.7 | |
| 0 | 15 | 0 | 11 | 17.36 | 27.46 | -46.76 | 69.54 | 0.7444 | -514.0 | -504.7 | |
| 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. | |