| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.64 | 19.08 | 1.13 | 12.35 | -9.84 | 18.50 | 40.18 | 263.06 | 0.6412 | 226.7 | 292.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.25 | 0.00 | 1.57 | -8.62 | 23.34 | 45.02 | 265.01 | 0.7044 | 781.0 | 647.0 | |
| 1.21 | 2.34 | 0.84 | 1.61 | -9.30 | 22.72 | 44.40 | 264.05 | 0.6966 | 648.4 | 557.7 | |
| 0.43 | 1.65 | 0.29 | 1.11 | -8.30 | 21.52 | 43.21 | 265.55 | 0.6819 | -712.6 | -630.7 | |
| 0.00 | 1.13 | 0.00 | 0.76 | -9.10 | 21.60 | 43.28 | 264.37 | 0.6826 | -652.0 | -460.7 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -9.41 | 18.88 | 40.56 | 263.93 | 0.6474 | 637.0 | 510.6 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -10.25 | 18.84 | 40.52 | 262.62 | 0.6470 | 622.0 | 438.8 | |
| 0.00 | 1.39 | 0.00 | 0.90 | -9.97 | 18.64 | 40.32 | 263.06 | 0.6443 | 686.0 | 544.1 | |
| 0.00 | 0.69 | 0.00 | 0.44 | -9.98 | 17.77 | 39.45 | 263.02 | 0.6328 | 395.0 | 390.5 | |
| 0.00 | 1.13 | 0.00 | 0.72 | -10.02 | 17.58 | 39.26 | 262.95 | 0.6303 | 455.0 | 434.0 | |
| 0.00 | 1.30 | 0.00 | 0.82 | -10.14 | 16.51 | 38.19 | 262.74 | 0.6158 | 723.0 | 577.0 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -10.16 | 15.44 | 37.12 | 262.66 | 0.6012 | 599.0 | 490.7 | |
| 0.00 | 2.69 | 0.00 | 1.65 | -11.45 | 14.90 | 36.58 | 260.44 | 0.5946 | 617.0 | 560.1 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -11.33 | 8.29 | 29.97 | 259.78 | 0.4998 | -590.0 | -496.7 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -11.85 | 7.58 | 29.26 | 258.58 | 0.4901 | -695.0 | -551.8 | |
| 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. | |