| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.42 | 296.64 | 56.86 | 244.53 | 13.87 | 14.16 | 52.51 | 285.22 | 0.7996 | -376.1 | -171.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.74 | 62.57 | 11.07 | 54.34 | 12.97 | 16.64 | 54.99 | 283.75 | 0.8239 | -686.7 | -241.1 | |
| 0.00 | 0.52 | 0.00 | 0.45 | 13.49 | 16.50 | 54.84 | 284.39 | 0.8230 | -303.0 | -300.2 | |
| 2.67 | -1.00 | 2.29 | -1.00 | 13.11 | 16.16 | 54.50 | 283.97 | 0.8193 | -797.7 | 999999 | |
| 13.25 | 80.21 | 11.49 | 69.50 | 14.44 | 16.36 | 54.70 | 285.56 | 0.8227 | -675.9 | -122.2 | |
| 0.00 | 0.60 | 0.00 | 0.51 | 12.38 | 15.56 | 53.90 | 283.15 | 0.8127 | -473.0 | -448.6 | |
| 6.28 | -4.00 | 5.40 | -4.00 | 14.24 | 16.07 | 54.42 | 285.36 | 0.8197 | -796.2 | 999999 | |
| 1.20 | -4.00 | 1.03 | -4.00 | 13.94 | 15.92 | 54.26 | 285.02 | 0.8178 | -615.9 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.61 | 13.43 | 15.69 | 54.03 | 284.43 | 0.8151 | -413.0 | -358.1 | |
| 1.03 | 1.98 | 0.87 | 1.67 | 12.84 | 15.34 | 53.68 | 283.74 | 0.8110 | -740.4 | -670.0 | |
| 0.00 | 1.72 | 0.00 | 1.41 | 9.57 | 14.31 | 52.65 | 279.78 | 0.7977 | -570.0 | -424.0 | |
| 3.61 | 26.85 | 3.05 | 22.50 | 13.51 | 15.30 | 53.64 | 284.57 | 0.8113 | -771.6 | -648.7 | |
| 0.00 | 1.89 | 0.00 | 1.60 | 13.93 | 15.39 | 53.73 | 285.08 | 0.8127 | -458.0 | -521.9 | |
| 3.70 | -11.00 | 3.10 | -11.00 | 13.61 | 15.02 | 53.37 | 284.73 | 0.8087 | -876.6 | 999999 | |
| 3.36 | 11.53 | 2.81 | 9.66 | 14.16 | 15.00 | 53.34 | 285.41 | 0.8091 | -667.3 | -585.4 | |
| 2.41 | -14.00 | 2.01 | -14.00 | 14.35 | 14.81 | 53.15 | 285.67 | 0.8074 | -774.0 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.79 | 14.71 | 14.94 | 53.28 | 286.10 | 0.8092 | -488.0 | -407.1 | |
| 0.00 | 0.86 | 0.00 | 0.73 | 16.73 | 15.19 | 53.53 | 288.52 | 0.8145 | -479.0 | -428.0 | |
| 0.00 | 1.29 | 0.00 | 1.06 | 14.65 | 14.20 | 52.54 | 286.14 | 0.8017 | -702.0 | -604.3 | |
| 2.07 | 79.43 | 1.60 | 60.82 | 14.09 | 11.42 | 49.76 | 285.89 | 0.7721 | -665.7 | -56.6 | |
| 2.93 | -19.00 | 2.27 | -19.00 | 14.28 | 11.28 | 49.62 | 286.16 | 0.7710 | -770.5 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.66 | 14.51 | 10.92 | 49.27 | 286.52 | 0.7675 | -527.0 | -511.7 | |
| 4.91 | -19.00 | 3.72 | -19.00 | 13.74 | 10.37 | 48.71 | 285.62 | 0.7602 | 645.4 | 999999 | |
| 2.50 | -19.00 | 1.90 | -19.00 | 14.25 | 10.43 | 48.77 | 286.28 | 0.7617 | -836.0 | 999999 | |
| 0.34 | -19.00 | 0.26 | -19.00 | 13.75 | 10.00 | 48.35 | 285.70 | 0.7562 | 667.5 | 999999 | |
| 0.43 | 1.64 | 0.32 | 1.23 | 14.43 | 9.83 | 48.17 | 286.62 | 0.7554 | 330.2 | 173.3 | |
| 0.00 | 1.55 | 0.00 | 1.15 | 13.76 | 9.09 | 47.43 | 285.88 | 0.7461 | 371.0 | 248.3 | |
| 3.36 | 7.23 | 2.48 | 5.34 | 13.46 | 8.97 | 47.31 | 285.51 | 0.7442 | 719.9 | 510.0 | |
| 0.43 | 1.46 | 0.31 | 1.07 | 13.33 | 8.35 | 46.69 | 285.45 | 0.7370 | 602.4 | 521.2 | |
| 0.00 | 1.29 | 0.00 | 0.94 | 14.09 | 8.32 | 46.67 | 286.48 | 0.7381 | 358.0 | 275.8 | |
| 0.00 | 0.43 | 0.00 | 0.31 | 13.64 | 8.03 | 46.37 | 285.94 | 0.7339 | 623.0 | 598.2 | |
| 1.20 | 2.50 | 0.88 | 1.82 | 13.92 | 8.05 | 46.40 | 286.31 | 0.7347 | 676.2 | 567.0 | |
| 0.00 | 1.81 | 0.00 | 1.31 | 14.42 | 7.70 | 46.04 | 287.06 | 0.7316 | 658.0 | 530.1 | |
| 0.00 | 0.77 | 0.00 | 0.59 | 19.60 | 9.04 | 47.38 | 293.54 | 0.7585 | 516.0 | 418.8 | |
| 0.00 | 1.29 | 0.00 | 0.94 | 18.56 | 7.01 | 45.35 | 292.79 | 0.7339 | 575.0 | 442.1 | |
| 0.00 | 1.46 | 0.00 | 0.99 | 18.39 | 2.82 | 41.16 | 294.01 | 0.6861 | 636.0 | 410.9 | |
| 0.00 | 0.77 | 0.00 | 0.53 | 19.35 | 3.02 | 41.37 | 295.26 | 0.6919 | 597.0 | 539.1 | |
| 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. | |