| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.70 | 23.87 | 1.98 | 17.18 | -18.78 | 133.40 | 44.07 | 245.23 | 0.7275 | -64.6 | -95.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.98 | 0.00 | 1.47 | -18.60 | 135.36 | 46.03 | 246.16 | 0.7480 | 578.0 | 491.5 | |
| 0.00 | 1.44 | 0.00 | 1.07 | -18.92 | 135.19 | 45.87 | 245.69 | 0.7473 | 706.0 | 621.9 | |
| 2.70 | 4.69 | 1.98 | 3.44 | -18.33 | 134.71 | 45.39 | 246.30 | 0.7403 | 662.3 | 526.6 | |
| 0.00 | 1.89 | 0.00 | 1.38 | -18.27 | 134.42 | 45.09 | 246.28 | 0.7369 | 682.0 | 558.8 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -19.19 | 134.32 | 45.00 | 245.03 | 0.7389 | -525.0 | -364.5 | |
| 0.00 | 0.36 | 0.00 | 0.26 | -19.90 | 134.03 | 44.70 | 244.00 | 0.7382 | -440.0 | -316.0 | |
| 0.00 | 0.81 | 0.00 | 0.59 | -19.72 | 133.51 | 44.18 | 244.04 | 0.7320 | 483.0 | 381.4 | |
| 0.00 | 5.23 | 0.00 | 3.65 | -17.67 | 131.92 | 42.60 | 246.17 | 0.7073 | -638.0 | -598.3 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -20.22 | 132.47 | 43.14 | 242.98 | 0.7227 | -489.0 | -412.4 | |
| 0.00 | 0.99 | 0.00 | 0.71 | -20.74 | 132.47 | 43.15 | 242.30 | 0.7247 | -537.0 | -431.7 | |
| 0.00 | 1.17 | 0.00 | 0.82 | -18.00 | 131.54 | 42.22 | 245.58 | 0.7041 | -433.0 | -485.6 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -20.13 | 132.13 | 42.80 | 242.95 | 0.7186 | -508.0 | -501.0 | |
| 0.00 | 0.72 | 0.00 | 0.50 | -18.79 | 131.56 | 42.24 | 244.51 | 0.7073 | -588.0 | -507.5 | |
| 0.00 | 1.62 | 0.00 | 1.15 | -21.07 | 131.79 | 42.46 | 241.57 | 0.7187 | -570.0 | -415.6 | |
| 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. | |