| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.56 | 183.71 | 19.01 | 95.73 | 9.22 | 336.61 | -15.44 | 58.39 | 0.3097 | -688.8 | -368.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 0.87 | 7.54 | 342.01 | -10.04 | 52.60 | 0.2185 | -869.0 | -756.3 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 7.69 | 341.85 | -10.20 | 52.48 | 0.2222 | -816.0 | -566.9 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 7.87 | 339.40 | -12.64 | 57.54 | 0.2581 | -887.0 | -699.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 7.94 | 339.21 | -12.84 | 57.72 | 0.2614 | -824.0 | -628.2 | |
| 30.13 | 138.73 | 15.67 | 72.16 | 9.32 | 336.94 | -15.11 | 57.65 | 0.3058 | -1297.6 | -420.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.06 | 336.64 | -15.41 | 61.79 | 0.2998 | -940.0 | -686.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 7.48 | 336.31 | -15.73 | 64.02 | 0.3004 | 967.0 | 805.6 | |
| 6.43 | 18.73 | 3.34 | 9.75 | 8.21 | 336.25 | -15.80 | 61.91 | 0.3067 | -1051.0 | -735.9 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 8.18 | 335.84 | -16.21 | 62.60 | 0.3126 | -760.0 | -520.6 | |
| 0.00 | 2.99 | 0.00 | 1.58 | 9.35 | 333.95 | -18.10 | 61.94 | 0.3489 | -650.0 | -625.1 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 7.17 | 333.98 | -18.06 | 67.77 | 0.3338 | -742.0 | -543.9 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 10.44 | 333.03 | -19.01 | 60.40 | 0.3701 | 776.0 | 704.6 | |
| 0.00 | 2.44 | 0.00 | 1.30 | 10.19 | 332.98 | -19.06 | 61.06 | 0.3689 | 932.0 | 775.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 8.49 | 333.02 | -19.03 | 65.27 | 0.3566 | 636.0 | 496.4 | |
| 0.00 | 2.44 | 0.00 | 1.30 | 10.19 | 332.62 | -19.42 | 61.49 | 0.3741 | 862.0 | 786.0 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 12.55 | 330.96 | -21.09 | 58.16 | 0.4152 | 365.0 | 467.8 | |
| 0.00 | 2.17 | 0.00 | 1.18 | 12.77 | 330.74 | -21.31 | 57.96 | 0.4199 | 920.0 | 642.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 13.52 | 329.86 | -22.19 | 57.42 | 0.4375 | 758.0 | 602.6 | |
| 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. | |