| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.84 | 249.04 | 29.99 | 135.93 | -13.23 | 121.40 | -14.96 | 143.22 | 0.4206 | 459.0 | 271.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.62 | 212.84 | 11.74 | 115.69 | -13.20 | 122.24 | -14.12 | 144.62 | 0.4120 | 1334.4 | 354.0 | |
| 13.09 | -1.00 | 7.11 | -1.00 | -12.99 | 122.00 | -14.36 | 143.85 | 0.4114 | 1243.2 | 999999 | |
| 6.68 | -1.00 | 3.64 | -1.00 | -13.41 | 121.81 | -14.55 | 144.11 | 0.4185 | 967.1 | 999999 | |
| 1.76 | 4.22 | 0.96 | 2.31 | -13.56 | 120.97 | -15.39 | 142.79 | 0.4283 | 850.8 | 672.0 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -13.34 | 119.80 | -16.56 | 140.42 | 0.4371 | 413.0 | 482.0 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -13.25 | 119.55 | -16.81 | 139.87 | 0.4386 | 767.0 | 605.5 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -13.17 | 119.27 | -17.09 | 139.27 | 0.4404 | 554.0 | 499.1 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -15.53 | 117.87 | -18.49 | 140.44 | 0.4819 | -661.0 | -491.5 | |
| 2.90 | 4.83 | 1.62 | 2.70 | -13.43 | 117.40 | -18.96 | 136.71 | 0.4628 | -982.4 | -770.6 | |
| 0.00 | 1.67 | 0.00 | 0.93 | -13.14 | 117.26 | -19.10 | 136.07 | 0.4612 | -1001.0 | -899.5 | |
| 8.79 | 14.76 | 4.92 | 8.27 | -13.26 | 116.70 | -19.67 | 135.41 | 0.4685 | -972.7 | -740.8 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -15.08 | 116.13 | -20.23 | 137.28 | 0.4942 | -268.0 | -339.6 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -13.76 | 116.23 | -20.14 | 135.49 | 0.4789 | -763.0 | -665.2 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -15.15 | 115.93 | -20.44 | 137.10 | 0.4971 | -776.0 | -590.4 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -15.38 | 115.84 | -20.53 | 137.30 | 0.5005 | -660.0 | -417.4 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -14.38 | 115.80 | -20.56 | 135.83 | 0.4901 | -701.0 | -488.8 | |
| 0.00 | 1.85 | 0.00 | 1.05 | -13.99 | 115.15 | -21.22 | 134.35 | 0.4931 | -553.0 | -498.4 | |
| 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. | |