| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.42 | 137.88 | 26.49 | 86.45 | -13.26 | 119.91 | -32.39 | 121.74 | 0.6151 | 408.1 | 101.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.14 | 110.43 | 21.21 | 68.60 | -13.07 | 120.61 | -31.69 | 122.00 | 0.6057 | 928.8 | 276.1 | |
| 4.14 | -1.00 | 2.59 | -1.00 | -13.22 | 120.12 | -32.19 | 121.83 | 0.6126 | 538.3 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.72 | -13.56 | 119.85 | -32.46 | 122.09 | 0.6181 | -443.0 | -334.4 | |
| 0.00 | 1.58 | 0.00 | 1.01 | -12.66 | 118.55 | -33.76 | 119.83 | 0.6272 | -152.0 | -114.3 | |
| 1.41 | 8.10 | 0.91 | 5.26 | -14.95 | 118.05 | -34.26 | 122.62 | 0.6480 | -684.5 | -591.1 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -11.71 | 118.58 | -33.73 | 118.49 | 0.6209 | 648.0 | 562.2 | |
| 0.00 | 1.94 | 0.00 | 1.24 | -13.31 | 118.22 | -34.08 | 120.51 | 0.6353 | -784.0 | -591.4 | |
| 1.76 | -5.00 | 1.14 | -5.00 | -14.68 | 117.84 | -34.47 | 122.09 | 0.6485 | -730.7 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.67 | -12.66 | 118.07 | -34.24 | 119.48 | 0.6329 | -288.0 | -361.7 | |
| 0.00 | 1.23 | 0.00 | 0.80 | -14.08 | 117.72 | -34.59 | 121.20 | 0.6460 | 558.0 | 388.8 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -14.50 | 117.60 | -34.70 | 121.69 | 0.6500 | 177.0 | 116.3 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -15.80 | 116.97 | -35.33 | 122.95 | 0.6654 | -320.0 | -425.3 | |
| 0.00 | 1.14 | 0.00 | 0.75 | -13.56 | 116.90 | -35.40 | 119.91 | 0.6520 | -746.0 | -526.8 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -13.73 | 116.76 | -35.55 | 120.04 | 0.6547 | -662.0 | -582.5 | |
| 0.00 | 3.52 | 0.00 | 2.33 | -14.69 | 116.35 | -35.95 | 121.04 | 0.6652 | -769.0 | -632.3 | |
| 0.00 | 0.62 | 0.00 | 0.41 | -14.44 | 116.24 | -36.06 | 120.63 | 0.6648 | -676.0 | -508.9 | |
| 0.97 | 4.49 | 0.64 | 2.96 | -13.37 | 115.94 | -36.36 | 119.00 | 0.6618 | -743.0 | -591.0 | |
| 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. | |