| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.89 | 0.00 | 13.34 | 7.15 | 265.56 | -12.17 | 100.12 | 0.2310 | 232.0 | 307.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.49 | 280.32 | 2.60 | 276.23 | 0.0457 | -881.0 | -668.1 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 6.30 | 279.66 | 1.94 | 328.07 | 0.0638 | -939.0 | -741.2 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 3.34 | 279.01 | 1.28 | 275.89 | 0.0226 | -926.0 | -756.5 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 4.05 | 276.35 | -1.37 | 58.60 | 0.0281 | -902.0 | -703.6 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.84 | 276.32 | -1.40 | 66.02 | 0.0269 | -851.0 | -680.9 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 3.07 | 275.43 | -2.29 | 93.45 | 0.0401 | -893.0 | -688.5 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 9.34 | 269.77 | -7.95 | 51.85 | 0.1744 | 990.0 | 841.0 | |
| 0.00 | 2.36 | 0.00 | 1.19 | 8.63 | 269.10 | -8.62 | 57.33 | 0.1769 | 788.0 | 700.3 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 8.60 | 265.21 | -12.51 | 66.05 | 0.2355 | 858.0 | 691.3 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 9.01 | 261.60 | -16.13 | 69.38 | 0.2944 | 924.0 | 776.2 | |
| 0.00 | 3.45 | 0.00 | 1.79 | 8.98 | 261.31 | -16.42 | 69.80 | 0.2987 | 865.0 | 840.5 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 8.78 | 260.35 | -17.37 | 71.37 | 0.3128 | 712.0 | 555.9 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 9.82 | 260.23 | -17.49 | 68.34 | 0.3200 | 782.0 | 568.2 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 8.84 | 260.15 | -17.57 | 71.37 | 0.3162 | 752.0 | 601.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 1.47 | 259.52 | -18.20 | 95.05 | 0.3149 | 774.0 | 541.7 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 8.85 | 251.18 | -26.54 | 76.75 | 0.4554 | 718.0 | 654.8 | |
| 0.00 | 2.00 | 0.00 | 1.11 | 7.68 | 250.99 | -26.73 | 79.36 | 0.4554 | 800.0 | 633.7 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 7.70 | 250.75 | -26.98 | 79.38 | 0.4592 | 605.0 | 465.6 | |
| 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. | |