| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64 | 250 | 50 | 203 | -6.20 | 83.69 | 50.90 | 256.46 | 0.7926 | -262.4 | -72.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 77 | 8 | 70 | -4.52 | 88.76 | 55.98 | 260.07 | 0.8409 | -668.2 | -304.2 | |
| 7 | 54 | 6 | 47 | -6.16 | 86.85 | 54.07 | 257.68 | 0.8262 | -629.2 | -320.7 | |
| 9 | -2 | 8 | -2 | -5.71 | 86.79 | 54.00 | 258.18 | 0.8247 | -796.1 | 999999 | |
| 0 | 5 | 0 | 4 | -7.35 | 82.25 | 49.47 | 254.88 | 0.7831 | 485.0 | 394.6 | |
| 7 | 12 | 5 | 10 | -7.72 | 81.89 | 49.10 | 254.30 | 0.7804 | 637.1 | 523.2 | |
| 5 | 18 | 4 | 14 | -8.45 | 82.01 | 49.22 | 253.44 | 0.7838 | 570.8 | 544.4 | |
| 0 | 5 | 0 | 4 | -7.30 | 81.70 | 48.92 | 254.76 | 0.7772 | 785.0 | 653.9 | |
| 0 | 3 | 0 | 2 | -6.38 | 81.28 | 48.49 | 255.77 | 0.7701 | 524.0 | 450.1 | |
| 0 | 3 | 0 | 2 | -7.90 | 78.59 | 45.80 | 252.88 | 0.7454 | 354.0 | 193.3 | |
| 14 | 27 | 10 | 19 | -7.54 | 77.64 | 44.85 | 252.99 | 0.7335 | -838.6 | -459.0 | |
| 3 | 8 | 2 | 6 | -6.72 | 76.44 | 43.65 | 253.61 | 0.7169 | -909.6 | -691.3 | |
| 0 | 6 | 0 | 4 | -6.32 | 75.00 | 42.21 | 253.58 | 0.6985 | 616.0 | 438.2 | |
| 4 | 11 | 3 | 7 | -8.88 | 72.42 | 39.64 | 248.86 | 0.6782 | 801.0 | 569.0 | |
| 6 | 21 | 4 | 14 | -7.98 | 72.26 | 39.48 | 250.03 | 0.6722 | 972.2 | 751.4 | |
| 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. | |