| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.66 | 431.85 | 35.94 | 226.12 | 12.54 | 13.60 | 0.56 | 358.31 | 0.3234 | -1010.6 | -390.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.20 | 0.00 | 1.14 | 11.39 | 14.08 | 1.05 | 356.61 | 0.3045 | -179.0 | -144.6 | |
| 68.66 | 408.62 | 35.94 | 214.01 | 12.59 | 13.72 | 0.68 | 357.93 | 0.3242 | -1533.2 | -439.4 | |
| 0.00 | 1.76 | 0.00 | 0.91 | 9.51 | 12.67 | -0.36 | 1.31 | 0.2725 | 779.0 | 680.0 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 9.95 | 12.52 | -0.51 | 1.81 | 0.2800 | 759.0 | 685.8 | |
| 0.00 | 2.11 | 0.00 | 1.10 | 11.23 | 11.91 | -1.13 | 3.67 | 0.3020 | -740.0 | -510.9 | |
| 0.00 | 2.46 | 0.00 | 1.28 | 11.74 | 11.81 | -1.22 | 3.86 | 0.3105 | -849.0 | -759.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 12.34 | 11.38 | -1.65 | 5.05 | 0.3211 | -535.0 | -441.2 | |
| 0.00 | 2.20 | 0.00 | 1.14 | 11.27 | 11.02 | -2.01 | 6.54 | 0.3039 | 1012.0 | 780.9 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 11.43 | 10.86 | -2.17 | 6.97 | 0.3068 | 915.0 | 727.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.44 | 10.73 | -2.30 | 6.97 | 0.3238 | 789.0 | 622.4 | |
| 0.00 | 4.23 | 0.00 | 2.22 | 12.72 | 10.67 | -2.36 | 7.05 | 0.3286 | 1165.0 | 907.3 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 11.46 | 10.68 | -2.35 | 7.54 | 0.3078 | 792.0 | 647.1 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.93 | 10.55 | -2.48 | 7.73 | 0.3159 | 989.0 | 792.1 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 11.85 | 9.36 | -3.67 | 11.43 | 0.3178 | 747.0 | 588.2 | |
| 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. | |