| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.57 | 47.91 | 21.23 | 49.48 | 19.52 | 65.32 | 56.21 | 296.79 | 0.8784 | 113.9 | 77.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.26 | 14.48 | 0.30 | 16.66 | 19.07 | 69.25 | 60.15 | 294.90 | 0.9056 | 111.0 | -185.9 | |
| 7.20 | -1.00 | 8.26 | -1.00 | 18.82 | 69.04 | 59.94 | 294.71 | 0.9036 | -402.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.15 | 18.42 | 68.31 | 59.21 | 294.52 | 0.8977 | -471.0 | -435.8 | |
| 0.00 | 0.86 | 0.00 | 0.97 | 19.03 | 68.60 | 59.50 | 295.07 | 0.9011 | -552.0 | -505.8 | |
| 0.00 | 1.46 | 0.00 | 1.57 | 18.21 | 67.23 | 58.12 | 294.65 | 0.8895 | -423.0 | -409.2 | |
| 0.00 | 1.71 | 0.00 | 1.85 | 18.87 | 67.11 | 58.01 | 295.40 | 0.8903 | -517.0 | -384.1 | |
| 1.37 | 2.23 | 1.38 | 2.24 | 19.16 | 64.62 | 55.51 | 296.59 | 0.8727 | 460.6 | 368.9 | |
| 0.00 | 0.86 | 0.00 | 0.84 | 19.94 | 63.36 | 54.26 | 297.92 | 0.8655 | 391.0 | 357.8 | |
| 0.00 | 1.80 | 0.00 | 1.73 | 19.64 | 62.62 | 53.52 | 297.88 | 0.8588 | 157.0 | 196.9 | |
| 3.94 | 21.08 | 3.81 | 20.23 | 20.11 | 62.75 | 53.64 | 298.34 | 0.8613 | 488.8 | 463.9 | |
| 2.66 | -10.00 | 2.54 | -10.00 | 19.90 | 62.27 | 53.17 | 298.30 | 0.8569 | 703.4 | 999999 | |
| 5.14 | -10.00 | 4.94 | -10.00 | 20.26 | 62.35 | 53.24 | 298.67 | 0.8587 | 544.3 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.19 | 20.80 | 60.78 | 51.68 | 299.90 | 0.8482 | 544.0 | 400.1 | |
| 0.00 | 1.11 | 0.00 | 1.05 | 21.91 | 61.03 | 51.92 | 301.00 | 0.8542 | 519.0 | 427.3 | |
| 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. | |