| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.00 | 81.90 | 15.21 | 41.44 | -6.47 | 148.73 | 11.76 | 273.44 | 0.2042 | 521.7 | 145.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.62 | -7.71 | 150.91 | 13.94 | 266.99 | 0.2402 | -801.0 | -680.3 | |
| 14.91 | 29.91 | 7.59 | 15.22 | -7.20 | 150.22 | 13.25 | 269.19 | 0.2284 | 1157.4 | 778.9 | |
| 1.12 | 25.95 | 0.57 | 13.14 | -6.68 | 149.47 | 12.50 | 271.63 | 0.2160 | 1012.5 | 864.9 | |
| 2.24 | -3.00 | 1.14 | -3.00 | -6.83 | 149.44 | 12.47 | 270.94 | 0.2154 | 1259.4 | 999999 | |
| 0.95 | -3.00 | 0.48 | -3.00 | -6.54 | 149.13 | 12.16 | 272.39 | 0.2104 | 1162.5 | 999999 | |
| 7.50 | -3.00 | 3.79 | -3.00 | -6.34 | 148.76 | 11.79 | 273.48 | 0.2043 | 1178.7 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -5.85 | 148.20 | 11.23 | 276.24 | 0.1958 | 727.0 | 585.7 | |
| 0.00 | 1.12 | 0.00 | 0.56 | -4.72 | 146.97 | 10.00 | 283.46 | 0.1787 | -1055.0 | -899.5 | |
| 1.38 | 18.19 | 0.69 | 9.15 | -5.61 | 146.86 | 9.89 | 278.60 | 0.1737 | -1010.9 | -885.6 | |
| 0.00 | 1.12 | 0.00 | 0.56 | -6.21 | 146.84 | 9.87 | 275.20 | 0.1719 | 706.0 | 431.2 | |
| 1.90 | -9.00 | 0.95 | -9.00 | -5.29 | 146.79 | 9.82 | 280.52 | 0.1736 | -1181.0 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.73 | -5.88 | 145.17 | 8.20 | 278.71 | 0.1442 | -971.0 | -714.1 | |
| 0.00 | 0.69 | 0.00 | 0.34 | -5.18 | 144.26 | 7.29 | 285.14 | 0.1315 | -725.0 | -607.2 | |
| 0.00 | 1.29 | 0.00 | 0.64 | -5.85 | 143.27 | 6.31 | 281.80 | 0.1122 | -939.0 | -861.3 | |
| 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. | |