| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.01 | 342.94 | 52.60 | 201.89 | 16.17 | 24.46 | -31.79 | 70.14 | 0.5384 | -123.9 | -77.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.96 | 167.97 | 2.24 | 95.14 | 16.17 | 28.46 | -27.78 | 68.45 | 0.4833 | -1242.0 | -412.8 | |
| 3.33 | -1.00 | 1.88 | -1.00 | 15.89 | 28.40 | -27.85 | 69.05 | 0.4830 | -1374.0 | 999999 | |
| 14.15 | -1.00 | 8.01 | -1.00 | 16.16 | 28.18 | -28.07 | 68.63 | 0.4872 | -1193.5 | 999999 | |
| 17.12 | -1.00 | 9.71 | -1.00 | 15.84 | 27.98 | -28.27 | 69.37 | 0.4888 | -1155.3 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 18.26 | 26.95 | -29.29 | 65.28 | 0.5135 | -637.0 | -427.4 | |
| 0.00 | 3.96 | 0.00 | 2.28 | 16.64 | 26.80 | -29.45 | 68.41 | 0.5086 | -653.0 | -526.8 | |
| 11.71 | 14.96 | 6.73 | 8.59 | 16.20 | 26.73 | -29.52 | 69.28 | 0.5079 | -919.7 | -575.5 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 15.67 | 26.05 | -30.20 | 70.61 | 0.5155 | -722.0 | -535.2 | |
| 0.00 | 4.60 | 0.00 | 2.68 | 17.21 | 25.45 | -30.80 | 68.01 | 0.5295 | -785.0 | -514.2 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 15.46 | 25.57 | -30.68 | 71.21 | 0.5215 | -631.0 | -529.2 | |
| 0.00 | 4.15 | 0.00 | 2.43 | 16.41 | 24.89 | -31.36 | 69.73 | 0.5342 | -631.0 | -657.8 | |
| 0.00 | 3.24 | 0.00 | 1.91 | 17.35 | 24.68 | -31.57 | 68.11 | 0.5406 | -539.0 | -559.1 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 17.04 | 24.59 | -31.66 | 68.72 | 0.5406 | -709.0 | -546.1 | |
| 0.00 | 2.25 | 0.00 | 1.33 | 16.59 | 24.37 | -31.87 | 69.62 | 0.5419 | -616.0 | -516.8 | |
| 0.00 | 1.89 | 0.00 | 1.12 | 16.53 | 23.78 | -32.46 | 69.98 | 0.5498 | -101.0 | -198.3 | |
| 0.00 | 2.25 | 0.00 | 1.35 | 18.31 | 22.89 | -33.35 | 67.26 | 0.5681 | -654.0 | -544.1 | |
| 0.00 | 1.98 | 0.00 | 1.18 | 15.54 | 23.36 | -32.88 | 71.89 | 0.5524 | 887.0 | 774.7 | |
| 0.00 | 2.07 | 0.00 | 1.24 | 15.32 | 22.31 | -33.94 | 72.63 | 0.5663 | 675.0 | 647.4 | |
| 0.00 | 3.69 | 0.00 | 2.25 | 17.50 | 21.52 | -34.72 | 69.17 | 0.5834 | 882.0 | 740.5 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 17.04 | 21.55 | -34.70 | 69.94 | 0.5816 | 725.0 | 540.4 | |
| 0.00 | 1.98 | 0.00 | 1.21 | 17.34 | 21.37 | -34.88 | 69.51 | 0.5849 | 733.0 | 600.4 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 16.27 | 21.24 | -35.00 | 71.34 | 0.5834 | 867.0 | 761.9 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 15.74 | 21.04 | -35.21 | 72.31 | 0.5846 | 803.0 | 682.0 | |
| 1.08 | 2.52 | 0.67 | 1.55 | 17.22 | 20.53 | -35.71 | 70.00 | 0.5955 | 849.5 | 719.4 | |
| 5.77 | 7.57 | 3.53 | 4.64 | 15.74 | 20.61 | -35.63 | 72.43 | 0.5904 | 960.5 | 693.5 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 17.05 | 20.26 | -35.99 | 70.37 | 0.5986 | 555.0 | 453.1 | |
| 4.51 | 13.16 | 2.78 | 8.12 | 16.61 | 20.16 | -36.09 | 71.13 | 0.5987 | 928.3 | 737.2 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 18.41 | 19.70 | -36.54 | 68.36 | 0.6100 | 596.0 | 425.7 | |
| 0.90 | 40.10 | 0.56 | 25.02 | 16.85 | 19.67 | -36.58 | 70.88 | 0.6058 | 784.5 | 260.0 | |
| 0.00 | 0.81 | 0.00 | 0.51 | 17.25 | 19.58 | -36.67 | 70.27 | 0.6081 | 617.0 | 531.1 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 16.01 | 19.58 | -36.67 | 72.28 | 0.6048 | 855.0 | 748.4 | |
| 9.46 | 52.36 | 5.87 | 32.48 | 15.70 | 19.60 | -36.64 | 72.78 | 0.6037 | 1079.5 | 454.9 | |
| 11.53 | -29.00 | 7.18 | -29.00 | 16.56 | 19.42 | -36.83 | 71.44 | 0.6083 | 905.3 | 999999 | |
| 2.16 | -29.00 | 1.35 | -29.00 | 16.99 | 19.32 | -36.92 | 70.78 | 0.6107 | 450.1 | 999999 | |
| 2.52 | -29.00 | 1.58 | -29.00 | 16.37 | 18.94 | -37.30 | 71.88 | 0.6140 | 559.5 | 999999 | |
| 0.81 | -32.00 | 0.51 | -32.00 | 15.70 | 19.05 | -37.19 | 72.94 | 0.6110 | 521.1 | 999999 | |
| 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. | |