| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.75 | 141.98 | 52.85 | 256.97 | 18.92 | 165.15 | -70.93 | 68.47 | 0.9613 | -185.6 | -127.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.43 | 83.50 | 11.53 | 133.48 | 18.75 | 167.81 | -68.26 | 68.10 | 0.9494 | -723.0 | -146.1 | |
| 3.54 | -1.00 | 5.62 | -1.00 | 19.11 | 167.50 | -68.57 | 67.80 | 0.9513 | -304.2 | 999999 | |
| 0.88 | -1.00 | 1.48 | -1.00 | 19.20 | 166.52 | -69.56 | 67.92 | 0.9562 | 93.3 | 999999 | |
| 0.27 | -1.00 | 0.43 | -1.00 | 18.64 | 166.94 | -69.14 | 68.40 | 0.9536 | -410.3 | 999999 | |
| 0.00 | 1.06 | 0.00 | 1.72 | 18.39 | 166.89 | -69.18 | 68.67 | 0.9535 | -457.0 | -374.1 | |
| 1.59 | -1.00 | 2.69 | -1.00 | 18.78 | 166.17 | -69.91 | 68.43 | 0.9574 | 131.4 | 999999 | |
| 3.80 | 10.26 | 6.30 | 17.02 | 18.21 | 166.41 | -69.66 | 68.96 | 0.9556 | -323.8 | -126.1 | |
| 0.00 | 0.97 | 0.00 | 2.01 | 20.20 | 163.12 | -72.95 | 67.59 | 0.9716 | 305.0 | 328.7 | |
| 1.42 | 6.55 | 2.75 | 12.72 | 18.59 | 163.66 | -72.42 | 69.11 | 0.9682 | 513.7 | 414.6 | |
| 0.00 | 0.62 | 0.00 | 1.08 | 16.90 | 165.31 | -70.77 | 70.53 | 0.9595 | 61.0 | 67.7 | |
| 0.00 | 0.71 | 0.00 | 1.47 | 19.16 | 162.80 | -73.27 | 68.70 | 0.9720 | 349.0 | 287.9 | |
| 9.82 | 38.04 | 22.05 | 86.97 | 19.20 | 161.71 | -74.37 | 68.86 | 0.9761 | -27.1 | -202.9 | |
| 0.00 | 0.27 | 0.00 | 0.50 | 16.27 | 163.87 | -72.21 | 71.44 | 0.9654 | 184.0 | 240.3 | |
| 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. | |