| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.29 | 230.10 | 18.06 | 121.18 | 23.45 | 154.79 | 10.29 | 331.02 | 0.3412 | -705.1 | -416.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.54 | 0.00 | 1.36 | 24.50 | 157.23 | 12.72 | 327.49 | 0.3745 | -747.0 | -601.0 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 24.15 | 157.19 | 12.69 | 327.01 | 0.3697 | -756.0 | -545.4 | |
| 6.93 | 208.26 | 3.65 | 109.63 | 23.09 | 155.39 | 10.89 | 329.11 | 0.3399 | -1286.7 | -467.1 | |
| 27.36 | -3.00 | 14.41 | -3.00 | 23.32 | 155.08 | 10.58 | 330.18 | 0.3404 | -1428.9 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 26.35 | 155.35 | 10.84 | 333.92 | 0.3850 | -840.0 | -683.7 | |
| 0.00 | 2.28 | 0.00 | 1.19 | 22.49 | 154.16 | 9.65 | 331.04 | 0.3214 | -927.0 | -702.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 22.98 | 152.81 | 8.31 | 335.20 | 0.3185 | 772.0 | 622.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 25.47 | 152.61 | 8.10 | 338.86 | 0.3544 | -704.0 | -536.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 23.05 | 152.35 | 7.85 | 336.49 | 0.3164 | 730.0 | 543.7 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 24.69 | 152.42 | 7.92 | 338.40 | 0.3414 | -756.0 | -615.8 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 24.44 | 152.24 | 7.74 | 338.55 | 0.3365 | -782.0 | -597.2 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 21.18 | 149.86 | 5.35 | 341.29 | 0.2725 | 800.0 | 561.8 | |
| 0.00 | 1.67 | 0.00 | 0.88 | 26.78 | 150.03 | 5.53 | 346.20 | 0.3620 | 809.0 | 614.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 24.63 | 148.67 | 4.17 | 348.13 | 0.3228 | 803.0 | 624.5 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 25.02 | 147.93 | 3.42 | 350.43 | 0.3267 | 805.0 | 655.9 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 26.38 | 147.70 | 3.19 | 351.73 | 0.3483 | 644.0 | 445.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 26.17 | 146.56 | 2.05 | 354.59 | 0.3426 | 737.0 | 558.5 | |
| 0.00 | 1.75 | 0.00 | 0.96 | 31.39 | 142.80 | -1.70 | 3.42 | 0.4263 | 684.0 | 575.2 | |
| 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. | |