| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.38 | 265.94 | 62.02 | 340.07 | -8.30 | 249.08 | -65.57 | 101.47 | 0.9208 | 321.4 | -104.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.17 | 258.79 | 3.74 | 330.26 | -8.81 | 250.85 | -63.80 | 102.36 | 0.9095 | 518.1 | -95.8 | |
| 4.17 | -1.00 | 4.96 | -1.00 | -8.52 | 250.59 | -64.06 | 102.00 | 0.9109 | 576.9 | 999999 | |
| 0.82 | -1.00 | 0.99 | -1.00 | -8.24 | 249.96 | -64.69 | 101.57 | 0.9150 | 495.7 | 999999 | |
| 3.71 | -1.00 | 4.52 | -1.00 | -7.96 | 249.90 | -64.75 | 101.26 | 0.9150 | 652.1 | 999999 | |
| 1.63 | -1.00 | 2.01 | -1.00 | -8.40 | 249.54 | -65.11 | 101.67 | 0.9180 | 295.0 | 999999 | |
| 3.17 | -1.00 | 3.95 | -1.00 | -8.69 | 249.44 | -65.21 | 101.96 | 0.9190 | 253.2 | 999999 | |
| 5.62 | -1.00 | 7.03 | -1.00 | -8.27 | 249.21 | -65.44 | 101.47 | 0.9201 | 432.5 | 999999 | |
| 15.40 | -1.00 | 19.28 | -1.00 | -7.78 | 249.14 | -65.51 | 100.93 | 0.9200 | 620.8 | 999999 | |
| 0.00 | 2.90 | 0.00 | 3.87 | -9.83 | 247.87 | -66.78 | 102.88 | 0.9305 | -469.0 | -494.2 | |
| 0.00 | 0.72 | 0.00 | 0.98 | -10.10 | 247.67 | -66.97 | 103.13 | 0.9320 | -329.0 | -332.1 | |
| 1.90 | -1.00 | 2.45 | -1.00 | -7.81 | 248.45 | -66.20 | 100.84 | 0.9246 | 159.0 | 999999 | |
| 5.62 | -1.00 | 7.35 | -1.00 | -8.09 | 248.12 | -66.53 | 101.08 | 0.9270 | 43.9 | 999999 | |
| 4.17 | -1.00 | 5.74 | -1.00 | -9.64 | 247.14 | -67.51 | 102.56 | 0.9347 | -626.8 | 999999 | |
| 0.00 | 3.53 | 0.00 | 4.96 | -8.73 | 246.52 | -68.13 | 101.48 | 0.9375 | -260.0 | -240.2 | |
| 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. | |