| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.82 | 20.97 | 0.59 | 13.90 | -13.42 | 254.26 | -38.35 | 114.40 | 0.6634 | 395.1 | 259.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.74 | -13.01 | 258.00 | -34.61 | 115.84 | 0.6171 | 652.0 | 505.4 | |
| 0.00 | 3.45 | 0.00 | 2.17 | -12.67 | 257.82 | -34.78 | 115.22 | 0.6174 | 731.0 | 569.3 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -12.86 | 257.71 | -34.89 | 115.45 | 0.6198 | 819.0 | 665.8 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -12.33 | 257.53 | -35.07 | 114.54 | 0.6193 | 767.0 | 669.8 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -12.41 | 256.05 | -36.55 | 113.82 | 0.6380 | 679.0 | 549.9 | |
| 0.00 | 1.18 | 0.00 | 0.77 | -13.18 | 255.61 | -37.00 | 114.71 | 0.6472 | 748.0 | 640.9 | |
| 0.00 | 2.45 | 0.00 | 1.59 | -12.96 | 255.45 | -37.15 | 114.31 | 0.6481 | 624.0 | 588.8 | |
| 0.00 | 0.91 | 0.00 | 0.59 | -12.50 | 255.18 | -37.43 | 113.49 | 0.6492 | 693.0 | 528.8 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -12.60 | 255.08 | -37.52 | 113.58 | 0.6508 | 610.0 | 592.0 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -13.02 | 254.69 | -37.92 | 113.99 | 0.6576 | 477.0 | 360.5 | |
| 0.00 | 1.18 | 0.00 | 0.83 | -15.06 | 251.06 | -41.54 | 114.98 | 0.7088 | 383.0 | 367.1 | |
| 0.00 | 1.27 | 0.00 | 0.90 | -14.24 | 249.81 | -42.80 | 113.32 | 0.7194 | -780.0 | -697.1 | |
| 0.00 | 0.82 | 0.00 | 0.59 | -14.92 | 249.60 | -43.01 | 114.12 | 0.7244 | -604.0 | -498.1 | |
| 0.82 | 3.36 | 0.59 | 2.41 | -14.63 | 249.49 | -43.11 | 113.71 | 0.7244 | -728.3 | -617.6 | |
| 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. | |