| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.40 | 330.76 | 38.85 | 225.96 | 14.85 | 133.33 | 43.48 | 284.57 | 0.6892 | -546.4 | -239.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.43 | 297.33 | 30.74 | 205.55 | 15.35 | 134.12 | 44.27 | 285.25 | 0.7000 | -1168.8 | -312.1 | |
| 2.88 | -1.00 | 1.97 | -1.00 | 14.96 | 133.53 | 43.68 | 284.79 | 0.6924 | -1051.9 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.97 | 12.81 | 128.12 | 38.27 | 282.34 | 0.6204 | 741.0 | 559.2 | |
| 0.00 | 0.27 | 0.00 | 0.17 | 9.99 | 126.81 | 36.96 | 277.87 | 0.6000 | 444.0 | 396.3 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 9.74 | 126.43 | 36.58 | 277.47 | 0.5946 | 526.0 | 466.3 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 9.32 | 126.34 | 36.49 | 276.77 | 0.5931 | 648.0 | 548.3 | |
| 0.00 | 1.53 | 0.00 | 0.94 | 9.70 | 126.16 | 36.31 | 277.42 | 0.5908 | 693.0 | 633.8 | |
| 1.62 | 21.45 | 0.99 | 13.06 | 9.96 | 125.85 | 36.00 | 277.89 | 0.5866 | 685.7 | 687.4 | |
| 1.17 | -8.00 | 0.71 | -8.00 | 10.30 | 125.74 | 35.89 | 278.49 | 0.5853 | 675.5 | 999999 | |
| 0.81 | -8.00 | 0.49 | -8.00 | 10.16 | 125.57 | 35.72 | 278.26 | 0.5828 | 900.3 | 999999 | |
| 6.49 | -8.00 | 3.95 | -8.00 | 9.98 | 125.51 | 35.66 | 277.96 | 0.5818 | 982.3 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.93 | 10.74 | 125.61 | 35.76 | 279.25 | 0.5838 | 641.0 | 463.5 | |
| 0.00 | 1.44 | 0.00 | 0.88 | 9.59 | 125.42 | 35.57 | 277.29 | 0.5804 | 837.0 | 756.0 | |
| 0.00 | 3.79 | 0.00 | 2.30 | 9.26 | 125.38 | 35.53 | 276.71 | 0.5797 | 943.0 | 660.2 | |
| 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. | |