| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.74 | 34.37 | 10.89 | 23.87 | 18.31 | 243.02 | -43.83 | 69.86 | 0.7020 | -145.3 | -77.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.69 | 6.78 | 4.44 | 4.50 | 18.13 | 245.97 | -40.88 | 69.36 | 0.6670 | -816.0 | -656.0 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 17.50 | 245.90 | -40.96 | 70.32 | 0.6663 | -736.0 | -615.0 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 17.86 | 245.75 | -41.10 | 69.82 | 0.6690 | -775.0 | -668.1 | |
| 0.00 | 1.99 | 0.00 | 1.33 | 17.75 | 245.53 | -41.33 | 70.04 | 0.6714 | -710.0 | -499.5 | |
| 0.00 | 1.54 | 0.00 | 1.02 | 17.56 | 245.49 | -41.36 | 70.33 | 0.6713 | -663.0 | -534.6 | |
| 0.00 | 1.18 | 0.00 | 0.79 | 17.82 | 245.16 | -41.69 | 70.03 | 0.6760 | -575.0 | -509.5 | |
| 3.35 | 6.51 | 2.33 | 4.53 | 18.38 | 242.80 | -44.05 | 69.84 | 0.7052 | -715.4 | -464.9 | |
| 0.00 | 0.99 | 0.00 | 0.72 | 18.94 | 240.97 | -45.88 | 69.49 | 0.7273 | 575.0 | 390.2 | |
| 0.00 | 0.90 | 0.00 | 0.65 | 18.63 | 240.95 | -45.91 | 69.93 | 0.7269 | 722.0 | 631.5 | |
| 0.00 | 1.08 | 0.00 | 0.78 | 19.05 | 240.70 | -46.15 | 69.41 | 0.7305 | 668.0 | 552.3 | |
| 3.62 | 3.89 | 2.60 | 2.79 | 18.13 | 240.98 | -45.88 | 70.60 | 0.7256 | 701.0 | 693.8 | |
| 2.08 | 3.35 | 1.52 | 2.44 | 18.89 | 240.20 | -46.66 | 69.74 | 0.7358 | 530.9 | 419.9 | |
| 0.00 | 1.27 | 0.00 | 0.93 | 19.16 | 240.10 | -46.76 | 69.39 | 0.7375 | 438.0 | 325.4 | |
| 0.00 | 2.17 | 0.00 | 1.59 | 18.68 | 239.90 | -46.96 | 70.09 | 0.7387 | 681.0 | 555.2 | |
| 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. | |