| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.46 | 48.32 | 7.59 | 25.17 | 16.83 | 40.54 | 2.74 | 351.85 | 0.3072 | -272.7 | -113.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.76 | 12.20 | 5.15 | 6.44 | 18.31 | 45.15 | 7.35 | 339.36 | 0.3460 | -940.2 | -731.7 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 15.95 | 41.37 | 3.57 | 348.05 | 0.2906 | -865.0 | -708.5 | |
| 0.00 | 3.25 | 0.00 | 1.69 | 16.17 | 41.28 | 3.48 | 348.51 | 0.2939 | -802.0 | -812.2 | |
| 2.80 | 8.31 | 1.45 | 4.32 | 16.62 | 41.25 | 3.46 | 348.89 | 0.3011 | -890.7 | -761.3 | |
| 0.00 | 2.26 | 0.00 | 1.17 | 15.76 | 40.89 | 3.09 | 349.49 | 0.2859 | -914.0 | -699.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 15.95 | 40.83 | 3.03 | 349.81 | 0.2889 | -825.0 | -643.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.54 | 40.67 | 2.87 | 350.09 | 0.2816 | -898.0 | -788.2 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 15.79 | 40.67 | 2.87 | 350.24 | 0.2858 | -854.0 | -666.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 15.44 | 40.32 | 2.52 | 351.22 | 0.2791 | -902.0 | -714.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.49 | 38.36 | 0.57 | 358.14 | 0.2935 | 820.0 | 712.7 | |
| 0.00 | 4.70 | 0.00 | 2.43 | 16.49 | 37.25 | -0.54 | 1.78 | 0.2935 | 432.0 | 701.8 | |
| 0.00 | 2.53 | 0.00 | 1.30 | 15.35 | 37.10 | -0.70 | 2.46 | 0.2744 | 816.0 | 561.2 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 16.42 | 36.91 | -0.89 | 2.93 | 0.2927 | 778.0 | 568.4 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 16.77 | 36.43 | -1.37 | 4.40 | 0.2991 | 716.0 | 532.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 16.27 | 35.80 | -2.00 | 6.62 | 0.2916 | 976.0 | 782.2 | |
| 0.00 | 3.16 | 0.00 | 1.64 | 16.65 | 35.64 | -2.16 | 6.99 | 0.2983 | 858.0 | 690.6 | |
| 1.90 | 2.53 | 0.99 | 1.32 | 17.25 | 35.21 | -2.58 | 8.03 | 0.3092 | 918.6 | 850.3 | |
| 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. | |