| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65 | 323 | 35 | 177 | -5.57 | 81.21 | -22.99 | 118.44 | 0.4433 | -288.6 | -75.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 85 | 6 | 46 | -5.90 | 84.44 | -19.76 | 122.79 | 0.4017 | -1562.0 | -908.5 | |
| 4 | -1 | 2 | -1 | -5.35 | 84.21 | -19.99 | 121.32 | 0.4001 | -967.0 | 999999 | |
| 4 | -1 | 2 | -1 | -5.95 | 84.14 | -20.05 | 122.50 | 0.4061 | -1208.4 | 999999 | |
| 8 | 45 | 5 | 24 | -5.87 | 83.27 | -20.93 | 121.21 | 0.4173 | -1269.9 | -694.2 | |
| 8 | -4 | 4 | -4 | -5.97 | 82.97 | -21.23 | 121.03 | 0.4221 | -1025.3 | 999999 | |
| 4 | 12 | 2 | 7 | -6.52 | 82.31 | -21.89 | 121.34 | 0.4354 | -582.1 | -441.8 | |
| 0 | 4 | 0 | 2 | -6.86 | 81.91 | -22.28 | 121.53 | 0.4435 | -435.0 | -311.6 | |
| 3 | 7 | 1 | 4 | -4.74 | 81.96 | -22.24 | 117.32 | 0.4263 | -691.7 | -533.8 | |
| 0 | 4 | 0 | 2 | -6.22 | 81.86 | -22.34 | 120.22 | 0.4391 | -294.0 | -338.7 | |
| 4 | 13 | 2 | 7 | -3.80 | 80.76 | -23.44 | 114.14 | 0.4368 | 1038.5 | 714.4 | |
| 0 | 5 | 0 | 3 | -6.04 | 80.67 | -23.52 | 118.55 | 0.4538 | 437.0 | 507.5 | |
| 0 | 6 | 0 | 3 | -7.26 | 80.31 | -23.89 | 120.48 | 0.4680 | 1060.0 | 716.5 | |
| 0 | 6 | 0 | 3 | -4.02 | 80.37 | -23.83 | 114.21 | 0.4438 | 948.0 | 689.0 | |
| 0 | 13 | 0 | 7 | -6.46 | 80.18 | -24.02 | 118.85 | 0.4636 | 573.0 | 574.2 | |
| 0 | 5 | 0 | 3 | -4.74 | 79.48 | -24.71 | 114.83 | 0.4610 | 687.0 | 592.0 | |
| 0 | 13 | 0 | 7 | -5.77 | 78.83 | -25.37 | 116.21 | 0.4770 | 1072.0 | 806.4 | |
| 4 | 105 | 2 | 59 | -4.89 | 78.83 | -25.37 | 114.54 | 0.4712 | 1057.5 | 499.0 | |
| 8 | -17 | 5 | -17 | -5.12 | 78.43 | -25.77 | 114.60 | 0.4782 | 1332.3 | 999999 | |
| 6 | -17 | 4 | -17 | -5.53 | 78.23 | -25.96 | 115.20 | 0.4836 | 950.6 | 999999 | |
| 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. | |