| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.08 | 0.00 | 11.19 | 5.04 | 262.58 | -18.60 | 72.10 | 0.3314 | 45.5 | -10.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.63 | 0.00 | 0.82 | 6.12 | 273.92 | -7.26 | 49.65 | 0.1656 | -822.0 | -663.7 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 4.99 | 273.65 | -7.52 | 56.26 | 0.1575 | -1021.0 | -700.0 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 5.42 | 273.53 | -7.65 | 54.50 | 0.1635 | -916.0 | -778.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.18 | 271.12 | -10.06 | 62.55 | 0.1969 | -758.0 | -646.9 | |
| 0.00 | 2.53 | 0.00 | 1.28 | 2.19 | 270.03 | -11.14 | 78.77 | 0.1977 | -848.0 | -736.4 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -0.63 | 266.83 | -14.35 | 92.53 | 0.2492 | -848.0 | -648.8 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 8.19 | 260.26 | -20.91 | 68.02 | 0.3826 | 734.0 | 541.3 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 5.80 | 259.52 | -21.66 | 74.59 | 0.3825 | 793.0 | 680.6 | |
| 0.00 | 1.90 | 0.00 | 1.02 | 5.77 | 258.99 | -22.18 | 75.00 | 0.3906 | 758.0 | 658.9 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 5.84 | 256.49 | -24.69 | 76.23 | 0.4296 | 384.0 | 423.5 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 6.02 | 255.40 | -25.78 | 76.35 | 0.4469 | 605.0 | 449.6 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 0.02 | 254.46 | -26.72 | 89.94 | 0.4515 | 670.0 | 545.0 | |
| 0.00 | 2.08 | 0.00 | 1.16 | 4.25 | 254.04 | -27.14 | 80.73 | 0.4628 | 770.0 | 623.2 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 9.44 | 248.88 | -32.30 | 72.71 | 0.5542 | 655.0 | 569.2 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 9.75 | 248.44 | -32.73 | 72.36 | 0.5613 | 527.0 | 433.9 | |
| 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. | |