| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.01 | 275.15 | 23.42 | 137.20 | 9.66 | 56.72 | 0.07 | 352.31 | 0.1138 | -974.9 | -406.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.22 | 245.53 | 21.53 | 122.33 | 9.42 | 57.11 | 0.46 | 355.79 | 0.1082 | -1475.9 | -463.8 | |
| 0.00 | 0.60 | 0.00 | 0.30 | 7.34 | 56.78 | 0.13 | 358.22 | 0.0715 | -924.0 | -740.4 | |
| 2.15 | -1.00 | 1.07 | -1.00 | 9.25 | 56.57 | -0.08 | 0.78 | 0.1048 | -930.6 | 999999 | |
| 1.64 | 2.07 | 0.82 | 1.03 | 9.87 | 56.24 | -0.41 | 3.53 | 0.1159 | -882.6 | -864.8 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 10.11 | 56.09 | -0.56 | 4.64 | 0.1203 | -866.0 | -621.6 | |
| 0.00 | 0.86 | 0.00 | 0.43 | 9.63 | 56.09 | -0.56 | 4.99 | 0.1120 | -637.0 | -567.3 | |
| 0.00 | 15.67 | 0.00 | 7.86 | 12.12 | 55.09 | -1.57 | 9.86 | 0.1570 | 212.0 | 114.1 | |
| 0.00 | 0.86 | 0.00 | 0.43 | 8.98 | 54.83 | -1.82 | 17.51 | 0.1050 | 560.0 | 387.9 | |
| 0.00 | 1.21 | 0.00 | 0.60 | 10.34 | 51.38 | -5.28 | 36.23 | 0.1538 | -1021.0 | -899.2 | |
| 0.00 | 0.60 | 0.00 | 0.30 | 10.30 | 50.87 | -5.79 | 38.91 | 0.1587 | -879.0 | -672.6 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 10.30 | 50.59 | -6.06 | 40.20 | 0.1617 | -942.0 | -809.7 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 17.36 | 48.84 | -7.82 | 28.00 | 0.2777 | 809.0 | 575.4 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 13.04 | 48.20 | -8.46 | 40.02 | 0.2238 | 921.0 | 696.5 | |
| 0.00 | 1.38 | 0.00 | 0.70 | 12.49 | 47.11 | -9.54 | 45.11 | 0.2296 | 900.0 | 796.5 | |
| 0.00 | 0.69 | 0.00 | 0.35 | 11.70 | 45.48 | -11.18 | 52.10 | 0.2417 | 833.0 | 674.6 | |
| 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. | |