| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.53 | 0.00 | 11.04 | 11.08 | 179.03 | 20.42 | 287.46 | 0.3553 | -144.1 | -114.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.71 | 11.20 | 188.12 | 29.50 | 280.00 | 0.4925 | -736.0 | -600.1 | |
| 0.00 | 1.79 | 0.00 | 1.01 | 10.57 | 187.94 | 29.33 | 278.75 | 0.4891 | -712.0 | -563.8 | |
| 0.00 | 2.05 | 0.00 | 1.16 | 11.25 | 187.28 | 28.66 | 280.26 | 0.4800 | -712.0 | -557.0 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 10.87 | 187.10 | 28.48 | 279.49 | 0.4767 | -822.0 | -714.2 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 11.49 | 186.88 | 28.26 | 280.84 | 0.4744 | -672.0 | -585.5 | |
| 0.00 | 1.70 | 0.00 | 0.95 | 11.94 | 186.37 | 27.75 | 281.93 | 0.4676 | -771.0 | -641.8 | |
| 0.00 | 1.52 | 0.00 | 0.85 | 11.54 | 185.98 | 27.36 | 281.17 | 0.4609 | -811.0 | -650.3 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 5.72 | 184.94 | 26.32 | 268.26 | 0.4432 | -559.0 | -409.5 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 15.00 | 182.93 | 24.31 | 290.15 | 0.4253 | -702.0 | -561.7 | |
| 0.00 | 2.14 | 0.00 | 1.09 | 10.13 | 172.68 | 14.06 | 282.79 | 0.2464 | 912.0 | 597.0 | |
| 0.00 | 2.14 | 0.00 | 1.07 | 11.65 | 164.45 | 5.83 | 307.97 | 0.1268 | 875.0 | 693.8 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 12.02 | 164.40 | 5.78 | 310.46 | 0.1300 | 796.0 | 669.3 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 7.20 | 162.20 | 3.58 | 269.73 | 0.0623 | 970.0 | 863.7 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 16.49 | 161.14 | 2.52 | 345.32 | 0.1672 | 926.0 | 805.6 | |
| 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. | |