| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.24 | 390.65 | 37.30 | 234.56 | 12.33 | 13.75 | -28.96 | 56.97 | 0.5664 | -813.4 | -370.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.45 | 4.94 | 15.59 | -27.12 | 67.92 | 0.4921 | 754.0 | 587.2 | |
| 58.55 | 361.21 | 35.05 | 216.59 | 12.47 | 14.02 | -28.69 | 56.53 | 0.5641 | -1369.7 | -440.1 | |
| 0.26 | -2.00 | 0.16 | -2.00 | 12.25 | 13.55 | -29.16 | 57.29 | 0.5680 | -730.0 | 999999 | |
| 0.26 | -2.00 | 0.16 | -2.00 | 12.65 | 13.18 | -29.52 | 57.02 | 0.5754 | -759.3 | 999999 | |
| 0.97 | -2.00 | 0.59 | -2.00 | 12.61 | 12.69 | -30.02 | 57.50 | 0.5810 | -625.9 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.80 | 11.45 | 12.09 | -30.62 | 59.75 | 0.5801 | -543.0 | -420.0 | |
| 1.58 | 4.66 | 0.96 | 2.84 | 11.74 | 11.91 | -30.80 | 59.45 | 0.5843 | -279.7 | 222.8 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 10.52 | 11.91 | -30.80 | 61.32 | 0.5760 | 776.0 | 662.8 | |
| 0.00 | 5.71 | 0.00 | 3.48 | 11.38 | 11.74 | -30.97 | 60.14 | 0.5838 | -97.0 | -57.2 | |
| 0.00 | 1.76 | 0.00 | 1.07 | 10.86 | 11.52 | -31.19 | 61.11 | 0.5831 | 625.0 | 570.0 | |
| 0.00 | 1.14 | 0.00 | 0.69 | 10.64 | 11.47 | -31.24 | 61.48 | 0.5823 | 734.0 | 547.2 | |
| 0.62 | 2.02 | 0.38 | 1.23 | 10.96 | 11.36 | -31.35 | 61.07 | 0.5857 | 917.1 | 789.7 | |
| 0.00 | 3.96 | 0.00 | 2.43 | 11.29 | 11.07 | -31.64 | 60.80 | 0.5915 | 616.0 | 577.7 | |
| 0.00 | 1.58 | 0.00 | 0.97 | 11.58 | 10.96 | -31.75 | 60.45 | 0.5947 | 949.0 | 830.7 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 11.82 | 10.64 | -32.07 | 60.34 | 0.6002 | 602.0 | 503.2 | |
| 0.00 | 1.76 | 0.00 | 1.04 | 3.28 | 11.09 | -31.62 | 73.87 | 0.5470 | 782.0 | 696.8 | |
| 0.00 | 1.49 | 0.00 | 0.95 | 12.66 | 8.39 | -34.32 | 60.80 | 0.6324 | 649.0 | 500.6 | |
| 0.00 | 1.32 | 0.00 | 0.84 | 9.07 | 6.82 | -35.89 | 67.00 | 0.6312 | 719.0 | 585.5 | |
| 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. | |