| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102 | 749 | 55 | 393 | 2.55 | 271.60 | -19.02 | 94.45 | 0.3278 | 1720.8 | 672.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 675 | 17 | 353 | 2.28 | 272.96 | -17.66 | 95.70 | 0.3060 | 2176.1 | 713.9 | |
| 15 | -1 | 8 | -1 | 2.15 | 272.43 | -18.19 | 95.90 | 0.3150 | 1624.1 | 999999 | |
| 0 | 4 | 0 | 2 | -0.24 | 272.24 | -18.38 | 103.19 | 0.3253 | -366.0 | -277.1 | |
| 0 | 6 | 0 | 3 | 0.91 | 272.12 | -18.50 | 99.61 | 0.3232 | 834.0 | 650.5 | |
| 11 | -1 | 6 | -1 | 3.42 | 272.00 | -18.61 | 91.81 | 0.3202 | 1627.0 | 999999 | |
| 0 | 5 | 0 | 3 | 0.79 | 271.87 | -18.74 | 99.85 | 0.3276 | 570.0 | 525.6 | |
| 7 | -1 | 4 | -1 | 2.33 | 271.66 | -18.96 | 95.09 | 0.3274 | 1248.9 | 999999 | |
| 0 | 6 | 0 | 3 | 0.56 | 271.63 | -18.99 | 100.41 | 0.3323 | 653.0 | 468.5 | |
| 32 | -1 | 17 | -1 | 2.90 | 271.56 | -19.05 | 93.30 | 0.3280 | 1708.9 | 999999 | |
| 5 | -1 | 3 | -1 | 2.86 | 271.20 | -19.42 | 93.36 | 0.3341 | 1273.6 | 999999 | |
| 0 | 6 | 0 | 3 | 4.43 | 270.88 | -19.74 | 88.63 | 0.3384 | 550.0 | 548.6 | |
| 0 | 8 | 0 | 4 | 3.24 | 266.83 | -23.78 | 91.53 | 0.4045 | 826.0 | 651.9 | |
| 0 | 4 | 0 | 2 | 0.69 | 266.70 | -23.91 | 97.74 | 0.4108 | 893.0 | 791.9 | |
| 0 | 14 | 0 | 8 | 2.34 | 266.51 | -24.10 | 93.68 | 0.4106 | 784.0 | 617.8 | |
| 0 | 7 | 0 | 4 | 1.44 | 263.58 | -27.04 | 95.07 | 0.4581 | 788.0 | 537.2 | |
| 0 | 5 | 0 | 3 | 2.11 | 260.58 | -30.03 | 93.08 | 0.5030 | -666.0 | -581.0 | |
| 0 | 9 | 0 | 5 | 2.74 | 258.95 | -31.67 | 91.62 | 0.5267 | -805.0 | -647.3 | |
| 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. | |