| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.59 | 177.83 | 14.52 | 90.41 | 6.51 | 204.46 | -12.60 | 76.73 | 0.2243 | -607.4 | -370.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 5.08 | 0.00 | 2.58 | 10.84 | 206.31 | -10.75 | 55.51 | 0.2232 | -458.0 | -389.4 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 10.20 | 206.30 | -10.76 | 58.03 | 0.2175 | -874.0 | -707.8 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.22 | 206.37 | -10.69 | 76.12 | 0.1907 | -959.0 | -756.3 | |
| 0.00 | 3.54 | 0.00 | 1.79 | 7.16 | 205.63 | -11.42 | 72.48 | 0.2070 | -1108.0 | -902.3 | |
| 28.23 | 152.69 | 14.33 | 77.50 | 6.27 | 204.75 | -12.31 | 77.59 | 0.2180 | -1408.6 | -425.9 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 11.71 | 204.37 | -12.69 | 56.70 | 0.2584 | -373.0 | -310.0 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 7.89 | 203.16 | -13.90 | 72.43 | 0.2508 | -758.0 | -515.5 | |
| 0.36 | 2.27 | 0.19 | 1.16 | 7.12 | 202.29 | -14.77 | 76.20 | 0.2616 | -994.2 | -777.5 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 6.05 | 202.01 | -15.05 | 80.44 | 0.2630 | 737.0 | 573.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 5.77 | 201.86 | -15.20 | 81.56 | 0.2649 | 1010.0 | 910.3 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 6.20 | 201.84 | -15.21 | 79.97 | 0.2661 | 883.0 | 724.8 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 5.61 | 198.01 | -19.04 | 83.46 | 0.3283 | 843.0 | 692.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 5.91 | 197.78 | -19.28 | 82.62 | 0.3326 | 851.0 | 682.7 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 8.81 | 197.45 | -19.61 | 74.33 | 0.3459 | 645.0 | 488.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.53 | 197.40 | -19.66 | 75.14 | 0.3457 | 822.0 | 610.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 6.21 | 197.28 | -19.78 | 81.90 | 0.3413 | 798.0 | 701.7 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 7.03 | 196.03 | -21.03 | 80.00 | 0.3631 | 773.0 | 531.1 | |
| 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. | |