| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.87 | 54.42 | 19.70 | 62.28 | 13.78 | 348.29 | -65.24 | 78.14 | 0.9012 | 51.1 | 220.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.24 | 13.05 | 356.64 | -56.89 | 79.10 | 0.8331 | -437.0 | -433.3 | |
| 0.00 | 1.51 | 0.00 | 1.42 | 12.16 | 354.61 | -58.92 | 80.13 | 0.8518 | -594.0 | -459.4 | |
| 6.76 | 8.98 | 6.46 | 8.58 | 12.43 | 353.96 | -59.56 | 79.80 | 0.8575 | -450.2 | -316.1 | |
| 0.00 | 0.98 | 0.00 | 0.94 | 11.54 | 353.98 | -59.55 | 80.84 | 0.8576 | -314.0 | -256.5 | |
| 1.69 | 4.27 | 1.65 | 4.18 | 12.84 | 353.12 | -60.41 | 79.32 | 0.8648 | -281.1 | -54.9 | |
| 0.00 | 0.89 | 0.00 | 0.89 | 12.98 | 352.49 | -61.04 | 79.14 | 0.8701 | 317.0 | 304.2 | |
| 2.85 | 4.09 | 2.95 | 4.24 | 13.56 | 351.25 | -62.28 | 78.46 | 0.8803 | 414.8 | 371.4 | |
| 0.00 | 3.65 | 0.00 | 4.35 | 14.33 | 347.07 | -66.45 | 77.50 | 0.9115 | 619.0 | 484.4 | |
| 0.00 | 3.38 | 0.00 | 4.07 | 14.56 | 346.86 | -66.67 | 77.25 | 0.9130 | 87.0 | 147.5 | |
| 0.00 | 2.22 | 0.00 | 2.65 | 13.81 | 347.14 | -66.39 | 78.07 | 0.9112 | 386.0 | 443.4 | |
| 1.69 | 8.18 | 2.06 | 9.96 | 14.08 | 346.50 | -67.02 | 77.76 | 0.9155 | 523.8 | 434.8 | |
| 0.44 | -11.00 | 0.55 | -11.00 | 14.28 | 346.38 | -67.15 | 77.53 | 0.9163 | 346.0 | 999999 | |
| 0.00 | 1.42 | 0.00 | 1.73 | 13.50 | 346.60 | -66.93 | 78.39 | 0.9150 | 310.0 | 213.2 | |
| 0.00 | 3.20 | 0.00 | 3.97 | 14.43 | 346.05 | -67.48 | 77.36 | 0.9185 | 381.0 | 264.0 | |
| 0.71 | 4.98 | 0.90 | 6.29 | 14.79 | 345.65 | -67.88 | 76.95 | 0.9211 | 318.2 | 199.6 | |
| 1.69 | 3.38 | 2.29 | 4.58 | 14.36 | 343.85 | -69.68 | 77.35 | 0.9326 | 347.6 | 286.8 | |
| 2.04 | 3.02 | 2.84 | 4.19 | 14.12 | 343.37 | -70.16 | 77.59 | 0.9356 | 178.9 | 167.5 | |
| 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. | |