| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 33.58 | 0.00 | 17.34 | 8.31 | 137.34 | -2.93 | 8.95 | 0.2812 | -49.4 | -31.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.62 | 7.69 | 143.14 | 2.87 | 349.05 | 0.2628 | -810.0 | -719.5 | |
| 0.00 | 5.35 | 0.00 | 2.73 | 6.46 | 142.29 | 2.03 | 351.54 | 0.2398 | -503.0 | -661.3 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 6.04 | 142.05 | 1.79 | 352.29 | 0.2320 | -969.0 | -777.1 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 6.16 | 141.78 | 1.52 | 353.50 | 0.2335 | -870.0 | -736.2 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 6.00 | 141.78 | 1.52 | 353.42 | 0.2310 | -909.0 | -740.1 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 6.74 | 140.50 | 0.23 | 359.03 | 0.2420 | -925.0 | -718.8 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 6.83 | 140.29 | 0.02 | 359.90 | 0.2435 | -946.0 | -807.1 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 7.07 | 140.23 | -0.03 | 0.14 | 0.2477 | -863.0 | -805.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 7.71 | 136.18 | -4.08 | 15.35 | 0.2677 | 770.0 | 601.8 | |
| 0.00 | 4.92 | 0.00 | 2.57 | 10.91 | 135.72 | -4.54 | 14.06 | 0.3214 | 782.0 | 663.1 | |
| 0.00 | 1.47 | 0.00 | 0.78 | 12.61 | 135.18 | -5.09 | 14.34 | 0.3509 | 5.0 | -1.6 | |
| 0.00 | 2.76 | 0.00 | 1.42 | 7.79 | 134.46 | -5.80 | 21.20 | 0.2781 | 728.0 | 596.0 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 7.49 | 134.23 | -6.04 | 22.40 | 0.2748 | 869.0 | 726.3 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 12.25 | 133.93 | -6.33 | 17.97 | 0.3508 | 10.0 | 5.9 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 11.44 | 131.81 | -8.45 | 24.35 | 0.3509 | 9.0 | 8.3 | |
| 0.00 | 2.24 | 0.00 | 1.17 | 8.36 | 131.76 | -8.50 | 28.71 | 0.3058 | 1002.0 | 702.4 | |
| 0.00 | 1.47 | 0.00 | 0.76 | 8.14 | 130.77 | -9.50 | 31.85 | 0.3108 | 889.0 | 744.7 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 9.05 | 130.04 | -10.22 | 32.23 | 0.3300 | 841.0 | 602.2 | |
| 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. | |