| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.60 | 175.44 | 59.97 | 160.84 | 10.25 | 179.87 | -56.07 | 75.93 | 0.8435 | 42.5 | 40.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.20 | 94.93 | 16.99 | 83.91 | 9.90 | 181.22 | -54.72 | 76.06 | 0.8307 | -684.2 | -157.5 | |
| 11.39 | -1.00 | 10.07 | -1.00 | 9.43 | 181.17 | -54.77 | 76.62 | 0.8304 | -626.4 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.73 | 10.30 | 180.41 | -55.53 | 75.75 | 0.8390 | 263.0 | 262.6 | |
| 0.00 | 0.99 | 0.00 | 0.90 | 11.12 | 180.13 | -55.81 | 74.85 | 0.8430 | 117.0 | 126.7 | |
| 0.00 | 1.44 | 0.00 | 1.30 | 9.81 | 180.43 | -55.51 | 76.33 | 0.8380 | 432.0 | 363.8 | |
| 0.00 | 2.42 | 0.00 | 2.19 | 9.59 | 180.32 | -55.62 | 76.61 | 0.8387 | 418.0 | 395.1 | |
| 0.00 | 1.08 | 0.00 | 0.98 | 9.88 | 180.08 | -55.86 | 76.31 | 0.8413 | -60.0 | -95.8 | |
| 0.00 | 0.81 | 0.00 | 0.74 | 10.33 | 179.74 | -56.20 | 75.86 | 0.8452 | -240.0 | -171.7 | |
| 0.81 | 5.47 | 0.74 | 4.98 | 8.78 | 179.79 | -56.14 | 77.66 | 0.8422 | 503.0 | 356.4 | |
| 0.00 | 0.27 | 0.00 | 0.25 | 10.82 | 179.09 | -56.85 | 75.42 | 0.8518 | 560.0 | 485.0 | |
| 0.99 | 6.64 | 0.93 | 6.23 | 10.12 | 178.78 | -57.16 | 76.29 | 0.8534 | -296.4 | 239.9 | |
| 1.26 | 4.40 | 1.18 | 4.12 | 9.04 | 178.83 | -57.10 | 77.54 | 0.8513 | -229.4 | -51.3 | |
| 27.72 | 46.39 | 26.92 | 44.99 | 11.46 | 178.03 | -57.91 | 74.90 | 0.8620 | 617.5 | 323.2 | |
| 2.24 | 4.04 | 2.16 | 3.89 | 10.68 | 178.22 | -57.72 | 75.76 | 0.8592 | 677.6 | 567.2 | |
| 0.00 | 1.26 | 0.00 | 1.22 | 10.60 | 177.89 | -58.05 | 75.92 | 0.8619 | 423.0 | 432.1 | |
| 0.00 | 1.53 | 0.00 | 1.49 | 10.30 | 177.50 | -58.43 | 76.33 | 0.8648 | 601.0 | 517.0 | |
| 0.99 | 2.96 | 0.98 | 2.92 | 10.81 | 177.29 | -58.65 | 75.79 | 0.8673 | 449.6 | 366.9 | |
| 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. | |