| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.79 | 0.00 | 10.12 | 5.59 | 257.36 | 38.49 | 278.59 | 0.6238 | 450.9 | 335.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 1.01 | 4.37 | 273.30 | 54.43 | 274.96 | 0.8162 | -372.0 | -314.5 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 2.25 | 270.82 | 51.95 | 272.41 | 0.7898 | -555.0 | -488.5 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 5.25 | 258.08 | 39.21 | 277.58 | 0.6374 | 567.0 | 465.4 | |
| 0.00 | 1.09 | 0.00 | 0.69 | 1.96 | 257.67 | 38.80 | 272.41 | 0.6291 | 457.0 | 413.8 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 0.82 | 255.99 | 37.11 | 270.59 | 0.6056 | 613.0 | 567.2 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 6.86 | 256.30 | 37.43 | 280.46 | 0.6159 | 582.0 | 447.0 | |
| 0.00 | 0.82 | 0.00 | 0.51 | 9.29 | 256.03 | 37.16 | 284.43 | 0.6178 | 540.0 | 529.6 | |
| 0.00 | 1.00 | 0.00 | 0.62 | 6.25 | 255.14 | 36.27 | 279.73 | 0.5988 | 612.0 | 438.9 | |
| 0.00 | 0.91 | 0.00 | 0.56 | 6.19 | 254.83 | 35.96 | 279.70 | 0.5944 | 643.0 | 532.7 | |
| 0.00 | 2.17 | 0.00 | 1.35 | 9.88 | 255.06 | 36.19 | 285.70 | 0.6065 | 533.0 | 411.7 | |
| 0.00 | 0.82 | 0.00 | 0.51 | 9.33 | 254.99 | 36.12 | 284.83 | 0.6040 | 637.0 | 513.2 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 9.36 | 254.69 | 35.82 | 284.98 | 0.6000 | 597.0 | 636.2 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 4.28 | 248.30 | 29.43 | 277.65 | 0.4964 | 836.0 | 624.9 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 4.48 | 245.10 | 26.23 | 278.91 | 0.4478 | 622.0 | 486.4 | |
| 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. | |