| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.95 | 0.00 | 10.12 | 5.34 | 260.07 | 19.16 | 288.49 | 0.3423 | 228.9 | 261.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.59 | 5.56 | 274.38 | 33.47 | 279.49 | 0.5586 | -706.0 | -536.3 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 4.84 | 272.70 | 31.79 | 278.56 | 0.5329 | -554.0 | -499.2 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 5.73 | 272.04 | 31.12 | 280.40 | 0.5249 | -740.0 | -518.6 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 4.61 | 269.51 | 28.59 | 278.91 | 0.4848 | -629.0 | -594.7 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -0.02 | 268.64 | 27.73 | 269.27 | 0.4672 | -518.0 | -426.7 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 2.99 | 268.48 | 27.56 | 275.77 | 0.4664 | -692.0 | -504.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 3.46 | 265.57 | 24.66 | 277.48 | 0.4217 | 657.0 | 459.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 4.42 | 262.05 | 21.14 | 281.20 | 0.3681 | 634.0 | 552.6 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 11.22 | 258.12 | 17.21 | 303.03 | 0.3476 | 662.0 | 508.6 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 4.99 | 256.63 | 15.71 | 286.68 | 0.2829 | 853.0 | 627.8 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 9.47 | 254.91 | 14.00 | 303.58 | 0.2876 | 810.0 | 516.3 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 6.37 | 253.92 | 13.00 | 295.11 | 0.2481 | 867.0 | 696.7 | |
| 0.00 | 2.08 | 0.00 | 1.05 | 5.15 | 250.65 | 9.73 | 296.41 | 0.1889 | 1052.0 | 826.9 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 1.17 | 246.49 | 5.58 | 278.30 | 0.0986 | 895.0 | 803.7 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.54 | 244.75 | 3.84 | 328.29 | 0.1271 | 842.0 | 679.4 | |
| 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. | |