| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84 | 300 | 62 | 221 | -6.42 | 83.10 | 45.94 | 254.53 | 0.7407 | -406.2 | -26.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 72 | 3 | 58 | -4.30 | 88.52 | 51.37 | 259.20 | 0.7953 | -704.7 | -299.8 | |
| 11 | -1 | 9 | -1 | -4.57 | 88.49 | 51.33 | 258.85 | 0.7956 | -654.1 | 999999 | |
| 0 | 4 | 0 | 3 | -5.22 | 86.95 | 49.79 | 257.61 | 0.7810 | -470.0 | -432.4 | |
| 25 | 64 | 20 | 50 | -6.16 | 86.76 | 49.60 | 256.39 | 0.7813 | -960.2 | -341.0 | |
| -4 | -4 | -4 | -4 | -5.75 | 86.58 | 49.43 | 256.85 | 0.7784 | 999999 | 999999 | |
| 0 | 4 | 0 | 3 | -6.57 | 86.03 | 48.87 | 255.64 | 0.7747 | -460.0 | -448.9 | |
| 0 | 6 | 0 | 4 | -7.20 | 82.29 | 45.14 | 253.54 | 0.7356 | 630.0 | 443.6 | |
| 0 | 4 | 0 | 3 | -8.01 | 82.40 | 45.25 | 252.52 | 0.7396 | 164.0 | 209.5 | |
| 0 | 3 | 0 | 2 | -6.96 | 81.93 | 44.77 | 253.70 | 0.7307 | 425.0 | 486.4 | |
| 6 | 50 | 5 | 37 | -7.59 | 81.79 | 44.63 | 252.82 | 0.7313 | 923.8 | 729.8 | |
| 6 | -10 | 4 | -10 | -8.32 | 81.89 | 44.74 | 251.91 | 0.7350 | 700.4 | 999999 | |
| 0 | 4 | 0 | 3 | -7.11 | 80.36 | 43.20 | 252.89 | 0.7132 | 395.0 | 353.5 | |
| 0 | 6 | 0 | 4 | -7.76 | 78.05 | 40.89 | 251.00 | 0.6884 | -167.0 | -236.7 | |
| 20 | 40 | 14 | 27 | -7.23 | 77.47 | 40.31 | 251.46 | 0.6793 | -990.8 | -673.8 | |
| 0 | 7 | 0 | 4 | -6.31 | 74.85 | 37.69 | 251.53 | 0.6430 | 737.0 | 470.1 | |
| 0 | 6 | 0 | 4 | -9.01 | 73.30 | 36.15 | 246.73 | 0.6365 | 489.0 | 482.2 | |
| 5 | 11 | 3 | 7 | -8.79 | 72.50 | 35.34 | 246.56 | 0.6253 | 783.7 | 668.4 | |
| 7 | 17 | 4 | 11 | -7.89 | 72.26 | 35.10 | 247.77 | 0.6176 | 1207.7 | 880.2 | |
| 0 | 2 | 0 | 1 | -8.33 | 72.21 | 35.05 | 247.07 | 0.6193 | 651.0 | 677.5 | |
| 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. | |