| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.23 | 27.37 | 0.73 | 16.59 | -17.76 | 328.59 | -33.43 | 112.28 | 0.5667 | 307.9 | 224.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.50 | 0.00 | 0.87 | -20.11 | 333.31 | -28.72 | 119.28 | 0.5193 | 759.0 | 683.2 | |
| 0.00 | 2.11 | 0.00 | 1.20 | -14.39 | 333.92 | -28.10 | 108.76 | 0.4838 | 855.0 | 663.3 | |
| 0.79 | 5.28 | 0.45 | 2.98 | -13.57 | 333.96 | -28.06 | 107.12 | 0.4805 | 761.6 | 677.4 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -14.32 | 333.68 | -28.34 | 108.50 | 0.4870 | 694.0 | 552.5 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -15.80 | 332.25 | -29.77 | 110.71 | 0.5129 | 708.0 | 534.3 | |
| 0.00 | 2.20 | 0.00 | 1.26 | -13.59 | 332.55 | -29.48 | 106.58 | 0.5010 | -858.0 | -622.8 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -15.82 | 332.10 | -29.92 | 110.68 | 0.5150 | 721.0 | 556.7 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -13.43 | 332.32 | -29.70 | 106.17 | 0.5038 | -579.0 | -431.6 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -17.98 | 329.42 | -32.60 | 113.27 | 0.5601 | 703.0 | 579.0 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -17.85 | 329.37 | -32.65 | 113.03 | 0.5602 | 581.0 | 490.8 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -19.42 | 328.72 | -33.30 | 115.38 | 0.5753 | 593.0 | 485.8 | |
| 0.44 | 2.11 | 0.28 | 1.33 | -24.02 | 326.83 | -35.19 | 121.63 | 0.6205 | 749.2 | 605.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -18.74 | 328.23 | -33.79 | 114.01 | 0.5788 | 476.0 | 443.1 | |
| 0.00 | 1.32 | 0.00 | 0.81 | -18.91 | 327.42 | -34.60 | 113.92 | 0.5899 | 615.0 | 390.6 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -23.03 | 326.18 | -35.85 | 119.79 | 0.6233 | -655.0 | -521.6 | |
| 0.00 | 0.62 | 0.00 | 0.42 | -18.58 | 319.19 | -42.83 | 110.58 | 0.6906 | -610.0 | -535.1 | |
| 0.00 | 3.61 | 0.00 | 2.62 | -22.28 | 316.17 | -45.85 | 114.85 | 0.7340 | -607.0 | -430.3 | |
| 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. | |