| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.54 | 65.44 | 10.18 | 32.49 | 7.61 | 345.24 | 1.30 | 195.94 | 0.0526 | 21.2 | -190.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.96 | 0.00 | 1.48 | 7.06 | 352.13 | 8.19 | 270.36 | 0.1420 | -895.0 | -739.2 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 7.19 | 351.64 | 7.70 | 271.29 | 0.1336 | -1259.0 | -979.1 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 8.24 | 350.52 | 6.58 | 280.47 | 0.1158 | -853.0 | -731.7 | |
| 0.00 | 4.48 | 0.00 | 2.23 | 7.97 | 350.05 | 6.11 | 278.74 | 0.1072 | -957.0 | -800.8 | |
| 0.00 | 2.78 | 0.00 | 1.38 | 7.26 | 349.00 | 5.06 | 272.31 | 0.0879 | -1058.0 | -870.6 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 7.02 | 348.63 | 4.69 | 269.50 | 0.0815 | -873.0 | -596.8 | |
| 0.00 | 6.64 | 0.00 | 3.29 | 6.76 | 346.70 | 2.76 | 263.49 | 0.0484 | -842.0 | -644.1 | |
| 0.00 | 1.97 | 0.00 | 0.98 | 7.07 | 345.76 | 1.82 | 269.68 | 0.0316 | -815.0 | -661.5 | |
| 0.00 | 1.79 | 0.00 | 0.89 | 8.40 | 345.67 | 1.73 | 307.67 | 0.0379 | -1234.0 | -954.5 | |
| 6.10 | 9.50 | 3.02 | 4.71 | 8.55 | 345.37 | 1.43 | 316.27 | 0.0357 | -1094.0 | -715.1 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 10.31 | 344.08 | 0.14 | 357.55 | 0.0567 | 953.0 | 811.1 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 13.90 | 343.18 | -0.76 | 6.21 | 0.1199 | 959.0 | 708.5 | |
| 0.00 | 2.06 | 0.00 | 1.02 | 6.92 | 343.08 | -0.87 | 100.62 | 0.0154 | 763.0 | 560.8 | |
| 6.64 | 11.93 | 3.29 | 5.91 | 7.25 | 343.04 | -0.90 | 79.10 | 0.0159 | 1120.1 | 811.2 | |
| 7.80 | 9.86 | 3.87 | 4.89 | 6.83 | 342.47 | -1.48 | 99.76 | 0.0261 | 1111.7 | 808.3 | |
| 0.00 | 2.15 | 0.00 | 1.07 | 6.49 | 341.13 | -2.82 | 101.81 | 0.0501 | 1017.0 | 811.2 | |
| 0.00 | 2.51 | 0.00 | 1.25 | 8.56 | 339.09 | -4.86 | 72.59 | 0.0881 | 924.0 | 718.8 | |
| 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. | |