| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.95 | 191.04 | 18.11 | 102.42 | 19.64 | 104.01 | -11.69 | 30.25 | 0.3818 | -876.5 | -405.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.90 | 111.47 | -4.23 | 12.45 | 0.3253 | -834.0 | -607.5 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 23.03 | 109.03 | -6.67 | 15.57 | 0.4001 | -759.0 | -611.0 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.20 | 107.89 | -7.81 | 27.28 | 0.2875 | -864.0 | -677.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 18.58 | 106.17 | -9.53 | 26.77 | 0.3500 | -817.0 | -521.2 | |
| 0.00 | 2.73 | 0.00 | 1.51 | 24.60 | 104.71 | -11.00 | 22.98 | 0.4462 | -811.0 | -655.1 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 22.32 | 104.05 | -11.65 | 26.64 | 0.4185 | -839.0 | -686.1 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 31.24 | 102.93 | -12.77 | 20.27 | 0.5477 | -686.0 | -531.2 | |
| 33.95 | 170.08 | 18.11 | 90.77 | 19.08 | 104.11 | -11.59 | 30.74 | 0.3732 | -1265.0 | -402.7 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 28.05 | 102.62 | -13.08 | 23.33 | 0.5066 | -749.0 | -603.6 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 26.23 | 101.89 | -13.82 | 26.22 | 0.4868 | -750.0 | -669.5 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 26.17 | 101.69 | -14.01 | 26.60 | 0.4872 | -751.0 | -600.2 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 25.15 | 101.61 | -14.09 | 27.81 | 0.4744 | -463.0 | -555.1 | |
| 0.00 | 1.19 | 0.00 | 0.70 | 30.04 | 100.74 | -14.96 | 24.36 | 0.5441 | -681.0 | -565.5 | |
| 0.00 | 1.45 | 0.00 | 0.85 | 29.77 | 100.61 | -15.10 | 24.79 | 0.5414 | -732.0 | -662.1 | |
| 0.00 | 1.19 | 0.00 | 0.70 | 29.26 | 100.44 | -15.27 | 25.49 | 0.5359 | -536.0 | -523.4 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 15.65 | 101.21 | -14.49 | 42.59 | 0.3576 | 838.0 | 689.0 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 17.83 | 99.17 | -16.53 | 42.20 | 0.4050 | 877.0 | 624.3 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 18.39 | 98.70 | -17.01 | 42.02 | 0.4164 | 692.0 | 517.1 | |
| 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. | |