| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.99 | 0.00 | 14.34 | 18.49 | 357.99 | 6.91 | 333.23 | 0.2499 | -334.2 | -280.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.79 | 0.00 | 0.92 | 16.34 | 4.09 | 13.00 | 307.18 | 0.2722 | -852.0 | -571.7 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 23.67 | 3.84 | 12.75 | 324.93 | 0.3534 | -692.0 | -473.8 | |
| 0.00 | 3.14 | 0.00 | 1.62 | 18.08 | 2.52 | 11.43 | 315.67 | 0.2708 | -868.0 | -642.2 | |
| 0.00 | 2.24 | 0.00 | 1.15 | 18.06 | 2.06 | 10.97 | 316.74 | 0.2653 | -1013.0 | -794.1 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 18.03 | 1.80 | 10.71 | 317.33 | 0.2620 | -898.0 | -706.4 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 18.53 | 1.76 | 10.68 | 318.73 | 0.2676 | -904.0 | -682.6 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 19.27 | 0.31 | 9.23 | 324.52 | 0.2620 | -726.0 | -517.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.72 | 0.17 | 9.08 | 321.05 | 0.2402 | -864.0 | -730.6 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 19.55 | 0.27 | 9.18 | 325.30 | 0.2653 | -694.0 | -528.1 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 18.75 | 0.03 | 8.94 | 324.11 | 0.2522 | -1025.0 | -820.4 | |
| 0.00 | 2.42 | 0.00 | 1.24 | 18.13 | 359.93 | 8.84 | 322.85 | 0.2430 | -898.0 | -694.2 | |
| 0.00 | 2.15 | 0.00 | 1.10 | 18.35 | 359.94 | 8.86 | 323.37 | 0.2460 | -870.0 | -667.5 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 16.39 | 353.31 | 2.22 | 347.03 | 0.1666 | 853.0 | 721.4 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 18.86 | 352.76 | 1.68 | 352.26 | 0.2067 | 971.0 | 782.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 19.07 | 348.18 | -2.90 | 12.99 | 0.2140 | 1003.0 | 834.9 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 18.77 | 345.65 | -5.43 | 23.84 | 0.2228 | 890.0 | 676.5 | |
| 0.00 | 1.88 | 0.00 | 0.96 | 18.58 | 345.53 | -5.55 | 24.68 | 0.2208 | 905.0 | 782.5 | |
| 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. | |