| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.63 | 233.46 | 55.27 | 294.57 | 15.53 | 88.42 | 67.91 | 283.86 | 0.9211 | 450.2 | 219.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.86 | 160.15 | 32.91 | 203.33 | 14.87 | 88.62 | 68.11 | 283.15 | 0.9226 | 653.4 | 264.7 | |
| 0.00 | 1.51 | 0.00 | 2.03 | 17.28 | 90.00 | 69.49 | 285.78 | 0.9310 | 457.0 | 401.4 | |
| 0.00 | 0.53 | 0.00 | 0.62 | 11.89 | 86.29 | 65.78 | 279.80 | 0.9074 | -443.0 | -347.8 | |
| 11.11 | 24.79 | 14.38 | 32.21 | 16.97 | 89.12 | 68.61 | 285.44 | 0.9255 | 285.3 | -133.2 | |
| 0.00 | 0.71 | 0.00 | 0.89 | 17.06 | 88.33 | 67.82 | 285.52 | 0.9205 | 254.0 | 173.8 | |
| 0.00 | 1.33 | 0.00 | 1.66 | 17.28 | 88.08 | 67.57 | 285.76 | 0.9188 | 241.0 | 198.8 | |
| 0.00 | 3.11 | 0.00 | 4.04 | 18.73 | 89.18 | 68.67 | 287.34 | 0.9258 | -244.0 | -175.7 | |
| 4.62 | 23.82 | 5.64 | 29.39 | 17.28 | 87.57 | 67.07 | 285.75 | 0.9154 | 614.2 | 167.0 | |
| 0.00 | 7.47 | 0.00 | 8.91 | 16.56 | 86.98 | 66.47 | 284.96 | 0.9114 | 653.0 | 468.7 | |
| 0.00 | 2.04 | 0.00 | 2.42 | 16.27 | 86.78 | 66.27 | 284.64 | 0.9101 | 549.0 | 475.6 | |
| 0.00 | 0.71 | 0.00 | 0.88 | 18.59 | 87.94 | 67.43 | 287.19 | 0.9178 | -337.0 | -287.2 | |
| 2.04 | 3.38 | 2.34 | 3.86 | 15.69 | 85.79 | 65.28 | 283.99 | 0.9031 | 521.7 | 373.2 | |
| 0.00 | 0.27 | 0.00 | 0.33 | 18.89 | 88.10 | 67.60 | 287.51 | 0.9189 | -431.0 | -467.0 | |
| 0.00 | 0.80 | 0.00 | 0.93 | 17.39 | 86.30 | 65.79 | 285.87 | 0.9066 | 418.0 | 368.2 | |
| 0.00 | 0.80 | 0.00 | 0.86 | 13.58 | 83.90 | 63.39 | 281.60 | 0.8891 | -519.0 | -460.0 | |
| 0.00 | 0.44 | 0.00 | 0.50 | 17.03 | 85.06 | 64.56 | 285.47 | 0.8977 | 471.0 | 430.8 | |
| 0.00 | 0.71 | 0.00 | 0.80 | 17.66 | 85.33 | 64.83 | 286.17 | 0.8998 | 270.0 | 315.1 | |
| 0.00 | 0.89 | 0.00 | 0.91 | 13.95 | 82.24 | 61.73 | 281.99 | 0.8758 | -448.0 | -415.6 | |
| 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. | |