| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.94 | 302.04 | 34.28 | 185.47 | -1.47 | 155.17 | 35.31 | 258.47 | 0.5919 | 845.5 | 331.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.20 | 270.50 | 23.53 | 166.61 | -1.50 | 155.48 | 35.62 | 258.55 | 0.5963 | 1144.9 | 342.1 | |
| 1.05 | -1.00 | 0.64 | -1.00 | -1.40 | 154.89 | 35.03 | 258.49 | 0.5879 | 1174.6 | 999999 | |
| 3.78 | -1.00 | 2.31 | -1.00 | -1.54 | 154.74 | 34.89 | 258.20 | 0.5863 | 1140.7 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.86 | -2.18 | 154.76 | 34.90 | 257.15 | 0.5887 | 222.0 | 235.2 | |
| 8.96 | 13.53 | 5.43 | 8.19 | -1.77 | 154.05 | 34.20 | 257.54 | 0.5776 | 941.0 | 673.8 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -0.08 | 153.60 | 33.75 | 260.26 | 0.5659 | 678.0 | 611.7 | |
| 3.95 | 6.24 | 2.37 | 3.74 | -0.41 | 153.49 | 33.64 | 259.66 | 0.5653 | 905.3 | 726.6 | |
| 0.00 | 1.58 | 0.00 | 0.93 | -0.25 | 152.06 | 32.21 | 259.37 | 0.5445 | 742.0 | 595.6 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -1.97 | 151.94 | 32.09 | 256.26 | 0.5487 | 592.0 | 438.1 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -0.89 | 151.54 | 31.68 | 258.01 | 0.5390 | -543.0 | -424.2 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -1.60 | 151.33 | 31.48 | 256.63 | 0.5387 | -560.0 | -432.8 | |
| 0.00 | 3.16 | 0.00 | 1.84 | -0.61 | 151.01 | 31.15 | 258.28 | 0.5304 | -797.0 | -619.4 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -1.70 | 150.01 | 30.15 | 255.78 | 0.5200 | -631.0 | -533.7 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -1.61 | 148.39 | 28.53 | 255.09 | 0.4961 | -690.0 | -564.0 | |
| 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. | |