| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.53 | 0.00 | 17.02 | 10.78 | 310.01 | 51.03 | 281.21 | 0.7798 | -7.9 | -157.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.09 | 0.00 | 3.54 | 11.23 | 313.99 | 55.01 | 281.37 | 0.8218 | -630.0 | -465.0 | |
| 0.00 | 1.45 | 0.00 | 1.24 | 10.91 | 313.63 | 54.65 | 281.01 | 0.8180 | -165.0 | -165.9 | |
| 0.00 | 0.27 | 0.00 | 0.23 | 11.17 | 312.58 | 53.60 | 281.42 | 0.8078 | -344.0 | -270.0 | |
| 0.00 | 1.18 | 0.00 | 0.98 | 11.31 | 312.36 | 53.37 | 281.61 | 0.8056 | -495.0 | -479.0 | |
| 0.00 | 0.91 | 0.00 | 0.74 | 10.32 | 311.64 | 52.65 | 280.44 | 0.7975 | -558.0 | -385.0 | |
| 0.00 | 1.00 | 0.00 | 0.79 | 9.15 | 310.36 | 51.38 | 279.04 | 0.7833 | -408.0 | -349.5 | |
| 0.00 | 0.82 | 0.00 | 0.64 | 9.07 | 309.95 | 50.97 | 278.98 | 0.7788 | -614.0 | -522.2 | |
| 0.00 | 1.54 | 0.00 | 1.21 | 8.17 | 309.63 | 50.65 | 277.83 | 0.7749 | -649.0 | -517.1 | |
| 0.00 | 3.00 | 0.00 | 2.34 | 10.08 | 309.57 | 50.59 | 280.30 | 0.7754 | -580.0 | -497.4 | |
| 0.00 | 0.91 | 0.00 | 0.68 | 10.24 | 307.22 | 48.23 | 280.75 | 0.7493 | 288.0 | 250.2 | |
| 0.00 | 1.54 | 0.00 | 1.14 | 10.48 | 306.80 | 47.81 | 281.11 | 0.7448 | 581.0 | 476.3 | |
| 0.00 | 0.73 | 0.00 | 0.53 | 10.21 | 306.56 | 47.57 | 280.77 | 0.7418 | 455.0 | 462.5 | |
| 0.00 | 0.27 | 0.00 | 0.20 | 11.51 | 305.87 | 46.88 | 282.61 | 0.7353 | 566.0 | 471.0 | |
| 0.00 | 1.00 | 0.00 | 0.73 | 11.73 | 305.69 | 46.70 | 282.95 | 0.7335 | 696.0 | 556.5 | |
| 0.00 | 1.00 | 0.00 | 0.73 | 12.13 | 305.78 | 46.80 | 283.47 | 0.7351 | 625.0 | 526.4 | |
| 0.00 | 1.09 | 0.00 | 0.78 | 13.46 | 304.51 | 45.53 | 285.51 | 0.7225 | 348.0 | 270.8 | |
| 0.00 | 0.73 | 0.00 | 0.52 | 14.97 | 304.82 | 45.83 | 287.51 | 0.7289 | 749.0 | 646.4 | |
| 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. | |