| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.06 | 64.25 | 6.00 | 34.85 | 16.46 | 102.81 | 3.70 | 351.21 | 0.4093 | -433.5 | -425.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.70 | 15.50 | 105.85 | 6.75 | 343.62 | 0.4036 | -901.0 | -714.4 | |
| 0.00 | 2.16 | 0.00 | 1.17 | 16.07 | 104.91 | 5.81 | 346.17 | 0.4085 | -1138.0 | -954.1 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 16.27 | 104.88 | 5.78 | 346.34 | 0.4114 | -833.0 | -802.3 | |
| 0.00 | 7.08 | 0.00 | 3.86 | 16.69 | 104.71 | 5.61 | 346.98 | 0.4173 | -854.0 | -758.3 | |
| 0.00 | 2.25 | 0.00 | 1.22 | 16.20 | 104.70 | 5.59 | 346.73 | 0.4097 | -847.0 | -765.7 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 16.95 | 104.50 | 5.40 | 347.59 | 0.4205 | -754.0 | -639.5 | |
| 0.00 | 2.85 | 0.00 | 1.55 | 16.88 | 104.22 | 5.12 | 348.18 | 0.4186 | -891.0 | -741.2 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 14.74 | 103.57 | 4.47 | 348.59 | 0.3829 | -852.0 | -700.3 | |
| 0.95 | 2.33 | 0.51 | 1.26 | 15.99 | 103.17 | 4.07 | 350.18 | 0.4015 | -1014.7 | -893.6 | |
| 10.11 | 27.38 | 5.49 | 14.86 | 16.61 | 103.03 | 3.93 | 350.77 | 0.4109 | -1032.0 | -567.7 | |
| 0.00 | 3.97 | 0.00 | 2.13 | 14.80 | 102.59 | 3.49 | 351.08 | 0.3810 | -616.0 | -620.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 17.88 | 102.24 | 3.14 | 352.99 | 0.4291 | -754.0 | -596.1 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 17.02 | 99.83 | 0.73 | 358.30 | 0.4126 | 784.0 | 689.5 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 14.78 | 99.67 | 0.57 | 358.54 | 0.3766 | 742.0 | 572.3 | |
| 0.00 | 2.07 | 0.00 | 1.11 | 15.23 | 99.48 | 0.38 | 359.03 | 0.3838 | 866.0 | 604.9 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 17.12 | 98.22 | -0.88 | 2.05 | 0.4142 | 890.0 | 810.1 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 16.60 | 97.44 | -1.66 | 3.93 | 0.4066 | 939.0 | 834.9 | |
| 0.00 | 1.81 | 0.00 | 1.01 | 20.33 | 96.74 | -2.36 | 4.77 | 0.4661 | 865.0 | 562.5 | |
| 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. | |