| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.85 | 146.88 | 27.87 | 181.53 | -13.24 | 229.42 | 66.20 | 256.38 | 0.9166 | 304.7 | 143.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.60 | 128.88 | 14.93 | 163.90 | -12.62 | 230.51 | 67.29 | 257.23 | 0.9247 | 500.4 | 177.3 | |
| 9.17 | -1.00 | 11.60 | -1.00 | -13.26 | 230.05 | 66.83 | 256.51 | 0.9219 | 554.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 1.34 | -12.65 | 229.64 | 66.43 | 257.14 | 0.9190 | 502.0 | 461.0 | |
| 1.08 | -1.00 | 1.34 | -1.00 | -13.09 | 229.56 | 66.34 | 256.66 | 0.9186 | 748.4 | 999999 | |
| 0.00 | 2.88 | 0.00 | 3.49 | -12.61 | 229.00 | 65.78 | 257.15 | 0.9146 | 633.0 | 566.2 | |
| 0.00 | 1.08 | 0.00 | 1.26 | -11.59 | 228.07 | 64.85 | 258.22 | 0.9076 | -266.0 | -212.1 | |
| 0.00 | 0.72 | 0.00 | 0.81 | -11.31 | 227.02 | 63.80 | 258.46 | 0.8998 | -213.0 | -220.4 | |
| 0.00 | 2.43 | 0.00 | 2.66 | -15.81 | 225.82 | 62.60 | 253.35 | 0.8935 | -298.0 | -194.5 | |
| 0.00 | 0.99 | 0.00 | 1.00 | -14.25 | 223.58 | 60.36 | 254.87 | 0.8747 | -446.0 | -373.7 | |
| 0.00 | 0.81 | 0.00 | 0.82 | -15.12 | 223.54 | 60.32 | 253.86 | 0.8751 | -470.0 | -353.8 | |
| 0.00 | 2.43 | 0.00 | 2.13 | -21.89 | 216.73 | 53.51 | 244.76 | 0.8269 | -501.0 | -416.5 | |
| 0.00 | 1.26 | 0.00 | 1.06 | -20.83 | 215.21 | 51.99 | 245.63 | 0.8107 | -603.0 | -477.2 | |
| 0.00 | 1.53 | 0.00 | 1.18 | -16.30 | 212.20 | 48.98 | 250.49 | 0.7706 | -634.0 | -518.9 | |
| 0.00 | 2.79 | 0.00 | 1.88 | -24.33 | 201.18 | 37.96 | 235.55 | 0.6820 | -766.0 | -563.1 | |
| 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. | |