| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.42 | 0.00 | 11.86 | 6.27 | 260.91 | -24.54 | 81.66 | 0.4157 | 408.8 | 375.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.68 | 3.58 | 278.82 | -6.64 | 85.91 | 0.1162 | -1005.0 | -867.7 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 4.26 | 276.13 | -9.33 | 82.76 | 0.1636 | -1003.0 | -778.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 1.47 | 274.11 | -11.35 | 98.04 | 0.1996 | -955.0 | -731.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 9.14 | 269.26 | -16.19 | 68.79 | 0.2966 | 1029.0 | 798.7 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 2.58 | 267.44 | -18.02 | 91.28 | 0.3104 | 716.0 | 587.9 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 9.63 | 265.14 | -20.32 | 71.21 | 0.3632 | 835.0 | 683.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 8.51 | 264.58 | -20.88 | 74.56 | 0.3672 | 755.0 | 505.0 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 8.75 | 261.29 | -24.17 | 75.75 | 0.4192 | 749.0 | 637.1 | |
| 0.00 | 2.18 | 0.00 | 1.19 | 8.66 | 261.02 | -24.43 | 76.10 | 0.4230 | 918.0 | 801.3 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 8.92 | 260.53 | -24.93 | 75.72 | 0.4314 | 713.0 | 594.0 | |
| 0.00 | 1.73 | 0.00 | 0.98 | 5.17 | 255.67 | -29.78 | 85.06 | 0.4985 | 860.0 | 646.1 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 5.49 | 250.87 | -34.59 | 84.86 | 0.5695 | 687.0 | 544.0 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 5.97 | 249.37 | -36.09 | 84.16 | 0.5910 | 561.0 | 452.6 | |
| 0.00 | 1.82 | 0.00 | 1.12 | 4.49 | 249.16 | -36.29 | 86.67 | 0.5933 | 625.0 | 467.8 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 6.40 | 247.49 | -37.97 | 83.61 | 0.6174 | 647.0 | 433.2 | |
| 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. | |