| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.94 | 0.00 | 12.65 | -13.00 | 225.64 | 26.99 | 240.08 | 0.5118 | -171.1 | 47.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.51 | -13.33 | 228.85 | 30.19 | 242.25 | 0.5552 | 609.0 | 525.9 | |
| 0.00 | 2.83 | 0.00 | 1.67 | -12.83 | 228.33 | 29.67 | 242.69 | 0.5454 | 626.0 | 567.8 | |
| 0.00 | 1.80 | 0.00 | 1.06 | -12.71 | 228.17 | 29.52 | 242.78 | 0.5426 | 897.0 | 668.0 | |
| 0.00 | 2.06 | 0.00 | 1.21 | -13.14 | 228.08 | 29.43 | 242.00 | 0.5441 | 594.0 | 513.2 | |
| 0.00 | 3.43 | 0.00 | 2.01 | -12.80 | 227.94 | 29.28 | 242.46 | 0.5401 | 923.0 | 763.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -11.85 | 223.97 | 25.32 | 240.83 | 0.4813 | -632.0 | -563.5 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -11.75 | 223.66 | 25.01 | 240.72 | 0.4765 | -748.0 | -639.0 | |
| 0.00 | 1.97 | 0.00 | 1.11 | -11.50 | 223.57 | 24.92 | 241.10 | 0.4735 | -749.0 | -681.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -11.96 | 223.41 | 24.76 | 240.09 | 0.4746 | -862.0 | -738.4 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -14.01 | 223.50 | 24.84 | 236.45 | 0.4911 | -393.0 | -390.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -13.49 | 223.34 | 24.68 | 237.22 | 0.4850 | -610.0 | -528.8 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -15.77 | 223.27 | 24.62 | 233.22 | 0.5026 | -592.0 | -473.8 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -16.55 | 221.72 | 23.07 | 230.18 | 0.4910 | -774.0 | -523.8 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -12.71 | 220.64 | 21.99 | 235.71 | 0.4439 | -684.0 | -507.6 | |
| 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. | |