| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.82 | 39.50 | 3.57 | 20.64 | 7.59 | 252.19 | 18.02 | 283.49 | 0.3168 | 458.3 | 511.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.58 | 6.43 | 255.53 | 21.35 | 278.58 | 0.3675 | -820.0 | -673.2 | |
| 1.00 | 2.63 | 0.53 | 1.39 | 7.35 | 254.03 | 19.85 | 281.74 | 0.3455 | -982.5 | -815.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 7.00 | 253.59 | 19.41 | 280.92 | 0.3374 | -985.0 | -760.7 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 7.03 | 253.30 | 19.12 | 281.17 | 0.3328 | -948.0 | -716.4 | |
| 2.00 | 7.72 | 1.05 | 4.04 | 8.06 | 252.53 | 18.36 | 284.69 | 0.3238 | 871.9 | 711.5 | |
| 1.82 | -5.00 | 0.95 | -5.00 | 7.97 | 252.40 | 18.22 | 284.51 | 0.3213 | 988.8 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 7.36 | 252.30 | 18.13 | 282.70 | 0.3177 | 766.0 | 600.9 | |
| 0.00 | 2.82 | 0.00 | 1.47 | 7.91 | 252.10 | 17.93 | 284.54 | 0.3164 | 950.0 | 711.7 | |
| 0.00 | 3.27 | 0.00 | 1.71 | 8.56 | 252.13 | 17.96 | 286.49 | 0.3194 | 860.0 | 726.6 | |
| 0.00 | 2.63 | 0.00 | 1.37 | 8.28 | 251.99 | 17.82 | 285.77 | 0.3160 | 882.0 | 551.9 | |
| 0.00 | 2.27 | 0.00 | 1.18 | 8.04 | 251.95 | 17.77 | 285.04 | 0.3143 | 1117.0 | 958.5 | |
| 2.00 | 10.45 | 1.04 | 5.43 | 7.26 | 251.33 | 17.16 | 282.97 | 0.3016 | 1135.6 | 846.3 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 6.38 | 250.59 | 16.42 | 280.49 | 0.2869 | 975.0 | 892.8 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 6.24 | 250.43 | 16.25 | 280.06 | 0.2838 | 907.0 | 724.5 | |
| 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. | |