| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.08 | 0.00 | 12.33 | 7.16 | 267.41 | -26.29 | 80.95 | 0.4469 | 209.4 | 184.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.51 | 4.74 | 279.78 | -13.92 | 82.71 | 0.2428 | -938.0 | -800.3 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 3.53 | 278.19 | -15.51 | 87.86 | 0.2683 | -784.0 | -601.6 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 0.85 | 278.18 | -15.52 | 97.84 | 0.2713 | -867.0 | -687.0 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 4.79 | 276.25 | -17.45 | 83.82 | 0.3019 | -878.0 | -676.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 3.24 | 274.61 | -19.09 | 88.99 | 0.3280 | -709.0 | -646.4 | |
| 0.00 | 2.82 | 0.00 | 1.57 | 10.66 | 267.60 | -26.10 | 72.38 | 0.4555 | 872.0 | 626.3 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 6.66 | 267.28 | -26.42 | 81.23 | 0.4491 | 585.0 | 480.5 | |
| 0.00 | 2.18 | 0.00 | 1.22 | 11.03 | 266.60 | -27.11 | 72.12 | 0.4718 | 878.0 | 618.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 11.30 | 266.29 | -27.42 | 71.73 | 0.4774 | 735.0 | 537.8 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 11.63 | 265.94 | -27.77 | 71.25 | 0.4838 | 608.0 | 524.7 | |
| 0.00 | 0.64 | 0.00 | 0.36 | 8.94 | 264.96 | -28.74 | 77.12 | 0.4892 | 435.0 | 338.7 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 1.37 | 264.11 | -29.60 | 92.64 | 0.4963 | 380.0 | 387.9 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 8.40 | 263.34 | -30.36 | 78.67 | 0.5120 | 702.0 | 538.3 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 9.28 | 260.53 | -33.17 | 77.80 | 0.5546 | 729.0 | 587.0 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 8.69 | 260.11 | -33.59 | 78.97 | 0.5593 | 530.0 | 355.2 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 9.42 | 260.00 | -33.70 | 77.70 | 0.5624 | 668.0 | 587.5 | |
| 0.00 | 1.00 | 0.00 | 0.69 | 6.11 | 249.64 | -44.07 | 84.38 | 0.6971 | 614.0 | 502.0 | |
| 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. | |