| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.79 | 173.78 | 13.18 | 88.96 | 6.56 | 204.47 | -14.26 | 77.95 | 0.2518 | -802.4 | -406.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.74 | 10.81 | 206.26 | -12.46 | 59.30 | 0.2476 | -932.0 | -682.5 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 11.02 | 205.81 | -12.92 | 59.43 | 0.2560 | -928.0 | -790.1 | |
| 1.82 | 4.27 | 0.93 | 2.17 | 7.10 | 205.60 | -13.12 | 74.72 | 0.2346 | -1084.2 | -828.8 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 11.56 | 204.76 | -13.96 | 59.51 | 0.2756 | -920.0 | -701.8 | |
| 23.97 | 154.44 | 12.25 | 78.95 | 6.29 | 204.67 | -14.05 | 78.81 | 0.2471 | -1392.7 | -435.2 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 9.10 | 204.52 | -14.21 | 68.25 | 0.2620 | -851.0 | -650.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 12.45 | 202.87 | -15.85 | 59.81 | 0.3099 | -729.0 | -453.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 6.99 | 202.40 | -16.33 | 77.76 | 0.2868 | -818.0 | -714.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 6.16 | 202.10 | -16.62 | 80.77 | 0.2894 | 763.0 | 577.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 5.97 | 202.08 | -16.65 | 81.42 | 0.2894 | 663.0 | 539.5 | |
| 0.00 | 2.00 | 0.00 | 1.06 | 8.12 | 197.93 | -20.79 | 76.88 | 0.3624 | 795.0 | 563.8 | |
| 0.00 | 1.73 | 0.00 | 0.92 | 8.85 | 197.30 | -21.43 | 75.30 | 0.3748 | 761.0 | 580.7 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 6.21 | 197.20 | -21.52 | 82.35 | 0.3696 | 863.0 | 782.6 | |
| 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. | |