| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.32 | 0.00 | 12.49 | 11.83 | 257.49 | -31.81 | 76.23 | 0.5338 | 493.4 | 378.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.02 | 16.26 | 268.76 | -20.55 | 60.57 | 0.3885 | -808.0 | -612.3 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 15.88 | 268.52 | -20.78 | 61.70 | 0.3892 | -884.0 | -702.5 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 16.43 | 259.13 | -30.17 | 67.48 | 0.5239 | 704.0 | 561.7 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 9.46 | 259.58 | -29.73 | 80.80 | 0.4975 | 731.0 | 500.9 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 16.55 | 258.37 | -30.93 | 67.65 | 0.5348 | 602.0 | 511.2 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 8.44 | 259.24 | -30.06 | 82.90 | 0.5013 | 721.0 | 675.8 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 8.64 | 259.01 | -30.29 | 82.52 | 0.5050 | 780.0 | 639.1 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 9.85 | 258.79 | -30.52 | 80.17 | 0.5098 | 767.0 | 525.5 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 8.54 | 258.77 | -30.54 | 82.76 | 0.5085 | 791.0 | 551.4 | |
| 0.00 | 0.82 | 0.00 | 0.47 | 10.46 | 258.15 | -31.16 | 79.11 | 0.5202 | 703.0 | 558.4 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 15.41 | 257.34 | -31.96 | 70.18 | 0.5446 | 672.0 | 459.8 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 12.35 | 256.07 | -33.23 | 76.10 | 0.5536 | 516.0 | 463.9 | |
| 0.00 | 1.90 | 0.00 | 1.14 | 10.88 | 254.85 | -34.46 | 78.99 | 0.5682 | 661.0 | 471.5 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 12.08 | 254.38 | -34.93 | 76.99 | 0.5768 | 581.0 | 394.6 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 5.02 | 254.54 | -34.76 | 89.34 | 0.5701 | 741.0 | 615.4 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 4.69 | 254.52 | -34.78 | 89.93 | 0.5706 | 598.0 | 435.1 | |
| 0.00 | 0.91 | 0.00 | 0.63 | 18.07 | 244.98 | -44.32 | 70.00 | 0.7091 | 579.0 | 497.4 | |
| 0.00 | 0.72 | 0.00 | 0.51 | 18.21 | 244.80 | -44.50 | 69.85 | 0.7115 | 426.0 | 386.4 | |
| 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. | |