| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.17 | 0.00 | 11.10 | 5.51 | 262.69 | -15.16 | 60.72 | 0.2857 | -116.9 | -78.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.64 | 273.82 | -4.03 | 35.59 | 0.1206 | -745.0 | -635.2 | |
| 0.00 | 3.71 | 0.00 | 1.85 | 5.30 | 273.67 | -4.18 | 38.31 | 0.1176 | -1083.0 | -849.9 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 5.12 | 273.30 | -4.55 | 41.68 | 0.1192 | -878.0 | -707.4 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 4.27 | 273.00 | -4.85 | 48.79 | 0.1125 | -976.0 | -829.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.48 | 272.21 | -5.64 | 36.95 | 0.1628 | -784.0 | -539.0 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 3.38 | 271.81 | -6.04 | 60.90 | 0.1207 | -908.0 | -624.4 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 1.47 | 269.06 | -8.79 | 80.69 | 0.1555 | -754.0 | -593.9 | |
| 0.00 | 3.98 | 0.00 | 2.09 | 8.17 | 260.35 | -17.50 | 64.57 | 0.3310 | 497.0 | 530.0 | |
| 0.00 | 0.36 | 0.00 | 0.20 | -0.46 | 254.35 | -23.50 | 91.24 | 0.4005 | 571.0 | 472.0 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 8.39 | 252.20 | -25.65 | 71.25 | 0.4542 | 778.0 | 617.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 9.32 | 252.06 | -25.79 | 69.40 | 0.4605 | 619.0 | 527.6 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 0.48 | 251.57 | -26.28 | 88.98 | 0.4447 | 73.0 | 81.7 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 8.73 | 249.44 | -28.41 | 72.16 | 0.4960 | 598.0 | 503.8 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 1.49 | 248.21 | -29.64 | 87.05 | 0.4970 | 645.0 | 576.0 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -0.15 | 246.31 | -31.54 | 90.35 | 0.5252 | 593.0 | 546.9 | |
| 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. | |