| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.90 | 31.14 | 1.96 | 20.54 | 16.19 | 27.47 | 36.08 | 301.23 | 0.6624 | 411.9 | 32.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.36 | 7.65 | 0.95 | 5.31 | 15.97 | 31.36 | 39.97 | 298.40 | 0.7044 | -569.3 | -607.9 | |
| 0.94 | 5.53 | 0.64 | 3.80 | 15.92 | 30.51 | 39.12 | 298.82 | 0.6949 | -715.5 | -542.9 | |
| 0.00 | 1.02 | 0.00 | 0.69 | 15.98 | 29.85 | 38.46 | 299.29 | 0.6880 | -670.0 | -564.4 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 17.05 | 25.94 | 34.55 | 303.29 | 0.6510 | 468.0 | 438.4 | |
| 0.00 | 1.11 | 0.00 | 0.71 | 16.60 | 24.99 | 33.60 | 303.37 | 0.6374 | 443.0 | 410.6 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 17.26 | 25.02 | 33.63 | 304.26 | 0.6422 | 552.0 | 444.9 | |
| 0.00 | 2.64 | 0.00 | 1.67 | 16.00 | 24.40 | 33.01 | 303.00 | 0.6267 | 492.0 | 403.5 | |
| 0.00 | 2.55 | 0.00 | 1.61 | 15.81 | 24.25 | 32.86 | 302.84 | 0.6237 | 790.0 | 617.9 | |
| 0.00 | 1.36 | 0.00 | 0.86 | 16.12 | 24.20 | 32.81 | 303.31 | 0.6252 | 628.0 | 515.9 | |
| 0.00 | 1.53 | 0.00 | 0.97 | 15.83 | 24.07 | 32.68 | 303.01 | 0.6218 | 856.0 | 638.6 | |
| 0.00 | 1.19 | 0.00 | 0.76 | 16.59 | 24.22 | 32.83 | 303.96 | 0.6287 | 484.0 | 341.8 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 16.71 | 23.98 | 32.59 | 304.30 | 0.6268 | 583.0 | 480.2 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 19.57 | 24.48 | 33.10 | 307.71 | 0.6527 | 577.0 | 506.6 | |
| 0.60 | 1.87 | 0.37 | 1.17 | 15.77 | 23.52 | 32.13 | 303.36 | 0.6150 | 855.6 | 728.5 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 16.20 | 23.12 | 31.73 | 304.27 | 0.6135 | 786.0 | 677.1 | |
| 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. | |