| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.19 | 204.75 | 48.69 | 258.55 | -14.66 | 116.86 | -63.93 | 109.04 | 0.9198 | 59.0 | -1.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.64 | 98.68 | 8.58 | 111.95 | -14.65 | 120.07 | -60.73 | 109.85 | 0.8991 | 733.8 | 193.3 | |
| 10.63 | -1.00 | 12.12 | -1.00 | -14.36 | 119.49 | -61.30 | 109.38 | 0.9026 | 592.2 | 999999 | |
| 0.00 | 2.37 | 0.00 | 2.84 | -14.87 | 118.32 | -62.48 | 109.60 | 0.9116 | -706.0 | -603.7 | |
| 0.00 | 2.20 | 0.00 | 2.56 | -13.93 | 118.78 | -62.02 | 108.72 | 0.9068 | 328.0 | 225.6 | |
| 2.20 | 2.99 | 2.59 | 3.52 | -13.82 | 118.37 | -62.43 | 108.49 | 0.9094 | 311.2 | 60.9 | |
| 1.05 | 4.66 | 1.26 | 5.58 | -13.64 | 117.98 | -62.82 | 108.20 | 0.9118 | 365.6 | 268.6 | |
| 1.23 | -6.00 | 1.48 | -6.00 | -13.54 | 117.68 | -63.12 | 108.02 | 0.9136 | 350.4 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.96 | -13.74 | 117.58 | -63.21 | 108.21 | 0.9146 | 376.0 | 336.6 | |
| 6.77 | 21.44 | 8.67 | 27.38 | -15.12 | 116.50 | -64.29 | 109.40 | 0.9239 | -622.4 | -457.9 | |
| 0.00 | 2.20 | 0.00 | 2.69 | -13.64 | 117.28 | -63.51 | 108.03 | 0.9164 | 126.0 | 42.2 | |
| 0.00 | 4.04 | 0.00 | 5.46 | -15.47 | 115.25 | -65.54 | 109.46 | 0.9320 | -457.0 | -262.9 | |
| 1.41 | 2.99 | 1.98 | 4.23 | -15.26 | 114.22 | -66.57 | 109.00 | 0.9377 | -432.1 | -332.2 | |
| 1.67 | 62.39 | 2.40 | 91.38 | -15.18 | 113.80 | -67.00 | 108.81 | 0.9400 | -418.0 | -93.4 | |
| 6.59 | -13.00 | 9.61 | -13.00 | -14.72 | 113.36 | -67.43 | 108.24 | 0.9418 | -468.4 | 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. | |