| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.28 | 28.11 | 2.06 | 17.63 | -15.28 | 246.23 | -30.87 | 126.25 | 0.6159 | -656.1 | -591.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.53 | -14.99 | 250.09 | -27.02 | 129.51 | 0.5709 | 653.0 | 568.1 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -14.95 | 247.47 | -29.63 | 126.90 | 0.5996 | -713.0 | -578.5 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -15.29 | 247.20 | -29.90 | 127.12 | 0.6053 | -709.0 | -650.0 | |
| 0.00 | 1.77 | 0.00 | 1.09 | -14.36 | 247.10 | -30.01 | 125.74 | 0.5991 | -757.0 | -597.2 | |
| 0.00 | 1.06 | 0.00 | 0.66 | -15.58 | 246.69 | -30.42 | 127.05 | 0.6133 | -474.0 | -554.6 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -15.76 | 246.44 | -30.67 | 127.06 | 0.6174 | -583.0 | -518.1 | |
| 0.00 | 1.50 | 0.00 | 0.94 | -15.21 | 246.38 | -30.72 | 126.28 | 0.6137 | -781.0 | -679.1 | |
| 0.71 | 2.12 | 0.44 | 1.32 | -14.64 | 246.33 | -30.77 | 125.44 | 0.6099 | -854.0 | -715.4 | |
| 0.00 | 4.51 | 0.00 | 2.85 | -15.96 | 245.93 | -31.17 | 126.88 | 0.6244 | -835.0 | -562.2 | |
| 1.86 | 10.79 | 1.17 | 6.79 | -15.31 | 245.97 | -31.14 | 126.04 | 0.6190 | -912.6 | -703.3 | |
| 0.00 | 1.15 | 0.00 | 0.73 | -15.81 | 245.74 | -31.37 | 126.51 | 0.6254 | -589.0 | -421.6 | |
| 0.71 | -10.00 | 0.45 | -10.00 | -15.12 | 245.78 | -31.32 | 125.63 | 0.6197 | -873.9 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -15.33 | 245.64 | -31.47 | 125.78 | 0.6229 | -683.0 | -599.2 | |
| 0.00 | 1.24 | 0.00 | 0.79 | -15.25 | 245.28 | -31.82 | 125.38 | 0.6262 | -845.0 | -691.0 | |
| 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. | |