| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.56 | 196.54 | 60.19 | 355.16 | 6.19 | 256.84 | 74.36 | 275.25 | 0.9616 | -243.2 | -86.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.31 | 176.57 | 16.01 | 331.16 | 6.02 | 257.88 | 75.40 | 275.10 | 0.9674 | 636.2 | -89.9 | |
| 20.76 | -1.00 | 38.55 | -1.00 | 6.03 | 257.29 | 74.81 | 275.09 | 0.9647 | -691.8 | 999999 | |
| 1.64 | 3.63 | 2.63 | 5.84 | 6.03 | 254.82 | 72.33 | 274.96 | 0.9525 | -448.5 | -419.9 | |
| 0.00 | 1.47 | 0.00 | 2.20 | 7.80 | 253.53 | 71.05 | 276.78 | 0.9451 | -228.0 | -207.2 | |
| 0.00 | 1.38 | 0.00 | 1.99 | 5.76 | 252.65 | 70.17 | 274.58 | 0.9405 | -508.0 | -372.7 | |
| 0.00 | 1.30 | 0.00 | 1.55 | 9.99 | 248.34 | 65.86 | 279.05 | 0.9118 | -151.0 | -207.1 | |
| 1.47 | 1.90 | 1.59 | 2.06 | 8.73 | 245.57 | 63.09 | 277.63 | 0.8911 | -334.2 | -391.8 | |
| 0.00 | 1.30 | 0.00 | 1.35 | 8.78 | 244.34 | 61.85 | 277.69 | 0.8812 | -529.0 | -425.1 | |
| 0.00 | 0.95 | 0.00 | 0.97 | 8.22 | 243.67 | 61.19 | 277.05 | 0.8758 | 311.0 | 194.5 | |
| 0.00 | 2.25 | 0.00 | 2.24 | 8.66 | 242.98 | 60.49 | 277.54 | 0.8699 | 547.0 | 387.0 | |
| 1.38 | 1.64 | 1.41 | 1.68 | 11.18 | 243.71 | 61.23 | 280.42 | 0.8763 | 261.4 | 383.3 | |
| 0.00 | 0.95 | 0.00 | 0.97 | 11.64 | 243.56 | 61.08 | 280.96 | 0.8752 | 450.0 | 388.8 | |
| 0.00 | 2.16 | 0.00 | 2.13 | 11.16 | 242.52 | 60.04 | 280.44 | 0.8663 | 601.0 | 517.4 | |
| 0.00 | 1.04 | 0.00 | 1.02 | 11.53 | 242.46 | 59.98 | 280.86 | 0.8659 | 504.0 | 425.1 | |
| 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. | |