| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.90 | 0.00 | 11.55 | -18.94 | 68.65 | -3.95 | 177.19 | 0.3212 | -122.0 | -107.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.67 | -19.84 | 82.66 | 10.06 | 210.95 | 0.3209 | 768.0 | 536.6 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -19.75 | 81.61 | 9.01 | 208.41 | 0.3111 | 742.0 | 606.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -19.57 | 81.53 | 8.93 | 208.52 | 0.3079 | 784.0 | 613.3 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -13.54 | 80.47 | 7.87 | 218.64 | 0.2141 | -699.0 | -615.3 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -13.39 | 80.43 | 7.83 | 218.97 | 0.2117 | -822.0 | -693.0 | |
| 0.00 | 1.27 | 0.00 | 0.64 | -12.59 | 80.07 | 7.47 | 220.24 | 0.1974 | -888.0 | -683.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -15.15 | 76.99 | 4.39 | 200.89 | 0.2082 | 851.0 | 548.5 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -16.69 | 76.28 | 3.68 | 195.63 | 0.2293 | 810.0 | 819.7 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -17.96 | 75.19 | 2.59 | 190.10 | 0.2463 | 544.0 | 336.9 | |
| 0.00 | 0.59 | 0.00 | 0.30 | -18.39 | 75.10 | 2.50 | 189.46 | 0.2532 | 281.0 | 529.3 | |
| 0.00 | 2.38 | 0.00 | 1.21 | -17.99 | 74.23 | 1.63 | 186.38 | 0.2445 | 979.0 | 821.7 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -16.36 | 63.37 | -9.23 | 144.39 | 0.2656 | -928.0 | -716.7 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -19.20 | 58.56 | -14.04 | 139.07 | 0.3513 | -1009.0 | -801.5 | |
| 0.00 | 1.61 | 0.00 | 0.85 | -18.17 | 57.40 | -15.20 | 134.78 | 0.3526 | -808.0 | -584.4 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -24.19 | 53.90 | -18.70 | 140.00 | 0.4570 | -988.0 | -849.4 | |
| 0.00 | 1.70 | 0.00 | 0.95 | -24.18 | 53.59 | -19.01 | 139.55 | 0.4600 | -879.0 | -727.8 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -28.67 | 40.54 | -32.06 | 132.50 | 0.6340 | -812.0 | -581.4 | |
| 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. | |