| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.08 | 160.44 | 41.30 | 100.23 | 34.08 | 267.89 | 6.47 | 351.18 | 0.6116 | -132.5 | 1.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.93 | 91.99 | 22.44 | 57.50 | 33.85 | 269.41 | 7.99 | 349.08 | 0.6115 | -1015.4 | -262.4 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 34.28 | 268.44 | 7.02 | 350.51 | 0.6150 | -388.0 | -205.8 | |
| 3.48 | 5.10 | 2.19 | 3.20 | 34.46 | 267.95 | 6.53 | 351.22 | 0.6164 | -570.7 | -485.6 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 33.10 | 267.21 | 5.79 | 351.82 | 0.5962 | 697.0 | 630.1 | |
| 0.00 | 0.93 | 0.00 | 0.57 | 33.06 | 267.00 | 5.58 | 352.11 | 0.5952 | 775.0 | 609.7 | |
| 0.00 | 2.12 | 0.00 | 1.31 | 33.46 | 266.84 | 5.42 | 352.43 | 0.6005 | 678.0 | 646.7 | |
| 1.53 | 2.29 | 0.95 | 1.42 | 33.53 | 266.53 | 5.11 | 352.88 | 0.6009 | 477.6 | 515.8 | |
| 0.00 | 1.10 | 0.00 | 0.70 | 35.20 | 266.49 | 5.07 | 353.33 | 0.6237 | 280.0 | 284.2 | |
| 0.00 | 7.73 | 0.00 | 4.83 | 34.34 | 266.18 | 4.76 | 353.54 | 0.6115 | -101.0 | -140.7 | |
| 0.00 | 0.85 | 0.00 | 0.53 | 33.71 | 266.15 | 4.73 | 353.44 | 0.6028 | 845.0 | 743.3 | |
| 1.53 | 37.12 | 0.95 | 23.14 | 33.97 | 265.81 | 4.39 | 353.97 | 0.6058 | 877.1 | 661.9 | |
| 4.16 | 5.61 | 2.62 | 3.52 | 34.86 | 265.56 | 4.14 | 354.47 | 0.6178 | 751.2 | 573.4 | |
| 19.45 | -11.00 | 12.15 | -11.00 | 34.45 | 265.26 | 3.84 | 354.80 | 0.6117 | 886.6 | 999999 | |
| 0.00 | 3.23 | 0.00 | 2.03 | 35.09 | 265.18 | 3.76 | 355.02 | 0.6203 | 689.0 | 490.5 | |
| 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. | |