| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.53 | 0.00 | 8.54 | -14.43 | 57.24 | -32.37 | 123.17 | 0.6205 | -68.8 | 105.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 1.73 | -15.13 | 59.96 | -29.65 | 126.40 | 0.5956 | 743.0 | 684.4 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -14.95 | 59.70 | -29.91 | 125.91 | 0.5971 | 721.0 | 699.8 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -12.64 | 60.03 | -29.58 | 122.87 | 0.5757 | 739.0 | 582.1 | |
| 0.00 | 1.67 | 0.00 | 1.01 | -11.87 | 59.21 | -30.41 | 121.00 | 0.5800 | -822.0 | -529.6 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -13.76 | 58.19 | -31.42 | 122.93 | 0.6056 | -557.0 | -470.1 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -13.44 | 57.77 | -31.84 | 122.12 | 0.6082 | -809.0 | -804.0 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -11.71 | 57.62 | -32.00 | 119.49 | 0.5983 | -556.0 | -409.4 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -13.40 | 57.30 | -32.31 | 121.70 | 0.6134 | -637.0 | -506.8 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -15.35 | 55.71 | -33.90 | 123.17 | 0.6449 | 720.0 | 458.5 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -15.10 | 55.61 | -34.00 | 122.75 | 0.6443 | 585.0 | 521.2 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -18.94 | 53.11 | -36.50 | 125.85 | 0.6965 | 470.0 | 382.4 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -13.52 | 53.89 | -35.72 | 119.38 | 0.6538 | -640.0 | -460.7 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -15.90 | 49.95 | -39.67 | 119.98 | 0.7111 | -537.0 | -581.3 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -18.40 | 44.95 | -44.67 | 120.20 | 0.7741 | -383.0 | -452.3 | |
| 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. | |