| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.58 | 30.08 | 6.06 | 18.70 | 13.88 | 90.67 | -36.89 | 75.64 | 0.6036 | 382.2 | 151.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.58 | 9.87 | 102.68 | -24.88 | 80.53 | 0.4220 | -766.0 | -644.0 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 14.54 | 97.44 | -30.11 | 72.34 | 0.5117 | -603.0 | -500.4 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 10.85 | 96.39 | -31.16 | 79.76 | 0.5185 | -651.0 | -526.8 | |
| 0.00 | 3.43 | 0.00 | 2.01 | 10.94 | 94.94 | -32.62 | 79.83 | 0.5398 | -567.0 | -536.5 | |
| 0.00 | 1.06 | 0.00 | 0.65 | 11.28 | 90.68 | -36.87 | 79.83 | 0.6001 | -674.0 | -598.9 | |
| 0.00 | 1.49 | 0.00 | 0.96 | 19.51 | 88.89 | -38.67 | 67.12 | 0.6415 | 725.0 | 557.8 | |
| 0.00 | 0.70 | 0.00 | 0.45 | 17.79 | 89.07 | -38.49 | 69.70 | 0.6341 | 537.0 | 452.2 | |
| 0.00 | 1.06 | 0.00 | 0.69 | 21.26 | 87.99 | -39.57 | 64.83 | 0.6582 | 638.0 | 510.0 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 16.66 | 89.23 | -38.33 | 71.41 | 0.6291 | 661.0 | 591.5 | |
| 0.00 | 0.79 | 0.00 | 0.51 | 17.66 | 88.90 | -38.66 | 69.96 | 0.6359 | 571.0 | 508.6 | |
| 0.00 | 0.88 | 0.00 | 0.56 | 16.44 | 89.04 | -38.52 | 71.82 | 0.6310 | 640.0 | 546.7 | |
| 9.58 | 13.98 | 6.06 | 8.84 | 13.24 | 89.11 | -38.44 | 76.87 | 0.6237 | 928.1 | 638.4 | |
| 0.00 | 0.97 | 0.00 | 0.62 | 13.33 | 88.66 | -38.90 | 76.80 | 0.6299 | 484.0 | 361.2 | |
| 0.00 | 1.41 | 0.00 | 0.90 | 13.50 | 88.03 | -39.53 | 76.64 | 0.6384 | 665.0 | 515.8 | |
| 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. | |