| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.75 | 85.68 | 15.17 | 43.75 | 20.08 | 109.96 | 0.07 | 0.06 | 0.2437 | 386.6 | 210.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.74 | 25.24 | 113.89 | 3.99 | 349.11 | 0.3351 | 797.0 | 684.2 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 24.33 | 113.36 | 3.47 | 349.98 | 0.3187 | 805.0 | 590.0 | |
| 4.55 | 18.64 | 2.32 | 9.52 | 19.98 | 112.24 | 2.35 | 350.87 | 0.2435 | -989.0 | -865.0 | |
| 2.80 | -3.00 | 1.43 | -3.00 | 20.16 | 112.05 | 2.16 | 351.71 | 0.2461 | -1033.8 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 26.46 | 111.82 | 1.93 | 355.04 | 0.3503 | 795.0 | 657.9 | |
| 3.85 | 6.30 | 1.97 | 3.22 | 20.07 | 111.66 | 1.77 | 353.12 | 0.2438 | -953.0 | -853.2 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 25.03 | 111.73 | 1.84 | 354.87 | 0.3267 | 758.0 | 601.4 | |
| 0.00 | 3.33 | 0.00 | 1.70 | 19.98 | 111.28 | 1.39 | 354.56 | 0.2415 | -1116.0 | -801.9 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 18.93 | 110.74 | 0.84 | 356.40 | 0.2230 | -856.0 | -682.5 | |
| 0.00 | 2.80 | 0.00 | 1.42 | 19.09 | 109.41 | -0.48 | 2.04 | 0.2254 | 687.0 | 653.3 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 19.80 | 109.40 | -0.49 | 1.94 | 0.2374 | 855.0 | 636.4 | |
| 0.00 | 4.46 | 0.00 | 2.27 | 19.52 | 109.12 | -0.77 | 3.13 | 0.2329 | 878.0 | 765.5 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 19.03 | 108.87 | -1.02 | 4.32 | 0.2248 | 933.0 | 755.5 | |
| 18.55 | 40.25 | 9.45 | 20.51 | 19.61 | 108.42 | -1.47 | 5.92 | 0.2354 | 1099.8 | 726.2 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 20.96 | 106.87 | -3.02 | 10.88 | 0.2619 | 837.0 | 601.2 | |
| 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. | |