| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.21 | 272.15 | 131.51 | 540.52 | 15.52 | 9.76 | -76.06 | 74.97 | 0.9671 | 171.4 | 151.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.07 | 0.00 | 3.49 | 18.70 | 12.51 | -73.32 | 71.66 | 0.9572 | -176.0 | -173.0 | |
| 19.95 | 102.01 | 28.94 | 148.26 | 14.86 | 15.46 | -70.36 | 75.64 | 0.9412 | -569.3 | -183.8 | |
| 0.00 | 2.07 | 0.00 | 3.17 | 14.09 | 14.33 | -71.49 | 76.48 | 0.9474 | 258.0 | 216.8 | |
| 0.00 | 2.07 | 0.00 | 3.69 | 14.79 | 11.51 | -74.32 | 75.75 | 0.9617 | 581.0 | 521.2 | |
| 4.23 | 129.82 | 7.78 | 278.28 | 14.75 | 10.95 | -74.87 | 75.79 | 0.9642 | 444.9 | 320.9 | |
| 0.00 | 1.12 | 0.00 | 2.42 | 16.50 | 8.42 | -77.40 | 73.98 | 0.9746 | 309.0 | 284.3 | |
| 4.84 | -5.00 | 9.53 | -5.00 | 15.05 | 9.78 | -76.05 | 75.49 | 0.9693 | 648.2 | 999999 | |
| 7.86 | -5.00 | 15.12 | -5.00 | 14.40 | 10.20 | -75.62 | 76.16 | 0.9675 | 171.6 | 999999 | |
| 6.56 | -5.00 | 14.82 | -5.00 | 16.30 | 7.80 | -78.03 | 74.18 | 0.9769 | 546.4 | 999999 | |
| 16.84 | -5.00 | 39.21 | -5.00 | 15.78 | 7.44 | -78.38 | 74.71 | 0.9782 | 350.7 | 999999 | |
| 0.00 | 1.64 | 0.00 | 5.45 | 17.66 | 3.47 | -82.35 | 72.72 | 0.9897 | -193.0 | -118.1 | |
| 0.00 | 1.81 | 0.00 | 4.05 | 14.81 | 8.11 | -77.72 | 75.71 | 0.9758 | -77.0 | -5.9 | |
| 0.00 | 0.26 | 0.00 | 0.72 | 16.57 | 5.33 | -80.50 | 73.87 | 0.9849 | 504.0 | 493.0 | |
| 4.15 | 13.82 | 13.64 | 45.57 | 17.24 | 3.75 | -82.08 | 73.15 | 0.9891 | 210.5 | 216.5 | |
| 0.78 | -14.00 | 2.47 | -14.00 | 16.82 | 3.99 | -81.83 | 73.58 | 0.9885 | 489.1 | 999999 | |
| 0.00 | 0.69 | 0.00 | 2.05 | 16.47 | 4.72 | -81.11 | 73.96 | 0.9866 | 499.0 | 469.0 | |
| 0.00 | 1.21 | 0.00 | 3.79 | 16.61 | 4.01 | -81.82 | 73.80 | 0.9885 | 575.0 | 500.5 | |
| 0.00 | 13.56 | 0.00 | 39.58 | 16.02 | 4.95 | -80.87 | 74.42 | 0.9860 | 290.0 | 270.8 | |
| 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. | |