| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.39 | 281.16 | 200.16 | 1027.33 | -7.24 | 241.28 | 81.58 | 262.09 | 0.9895 | -48.6 | 84.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.54 | 123.60 | 9.34 | 660.50 | -6.70 | 244.09 | 84.39 | 262.89 | 0.9965 | -382.7 | 186.4 | |
| 15.17 | -1.00 | 81.17 | -1.00 | -7.41 | 243.72 | 84.01 | 262.14 | 0.9960 | 36.8 | 999999 | |
| 0.00 | 6.36 | 0.00 | 20.61 | -4.83 | 240.40 | 80.69 | 264.45 | 0.9887 | 347.0 | 204.3 | |
| 4.36 | -1.00 | 24.60 | -1.00 | -8.82 | 243.85 | 84.14 | 260.74 | 0.9964 | -29.8 | 999999 | |
| 0.00 | 1.54 | 0.00 | 3.94 | -4.45 | 238.15 | 78.44 | 264.63 | 0.9819 | -3.0 | -2.5 | |
| 0.00 | 5.90 | 0.00 | 14.62 | -4.85 | 237.69 | 77.98 | 264.18 | 0.9805 | -274.0 | -182.0 | |
| 4.72 | 57.76 | 11.78 | 136.88 | -6.57 | 237.60 | 77.90 | 262.43 | 0.9808 | -284.5 | 11.7 | |
| 14.53 | -7.00 | 33.58 | -7.00 | -5.62 | 236.85 | 77.14 | 263.32 | 0.9778 | 284.3 | 999999 | |
| 12.26 | 61.12 | 29.52 | 146.56 | -7.93 | 237.08 | 77.37 | 261.00 | 0.9795 | -334.8 | -217.2 | |
| 0.00 | 1.45 | 0.00 | 3.24 | -6.38 | 236.23 | 76.52 | 262.48 | 0.9758 | -303.0 | -229.8 | |
| 0.00 | 1.09 | 0.00 | 1.96 | -5.24 | 233.25 | 73.55 | 263.34 | 0.9627 | 255.0 | 208.6 | |
| 5.81 | 17.98 | 10.17 | 31.49 | -4.99 | 232.74 | 73.04 | 263.55 | 0.9602 | -436.8 | -287.9 | |
| 0.00 | 0.73 | 0.00 | 1.28 | -5.89 | 232.81 | 73.11 | 262.62 | 0.9610 | -158.0 | -95.6 | |
| 0.00 | 3.63 | 0.00 | 6.25 | -5.74 | 232.44 | 72.74 | 262.74 | 0.9591 | -484.0 | -385.9 | |
| 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. | |