| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.29 | 91.82 | 23.71 | 76.02 | 19.80 | 64.71 | 46.80 | 301.13 | 0.8026 | 126.9 | 179.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 1.00 | 17.77 | 69.25 | 51.35 | 296.68 | 0.8345 | -413.0 | -376.2 | |
| 10.80 | 18.95 | 9.69 | 17.01 | 19.15 | 68.83 | 50.92 | 298.40 | 0.8359 | -634.9 | -199.7 | |
| 0.00 | 4.20 | 0.00 | 3.80 | 19.53 | 68.99 | 51.09 | 298.75 | 0.8386 | 263.0 | 161.6 | |
| 0.00 | 0.94 | 0.00 | 0.81 | 18.87 | 67.24 | 49.33 | 298.79 | 0.8212 | -611.0 | -520.2 | |
| 0.00 | 2.40 | 0.00 | 2.08 | 19.10 | 67.28 | 49.38 | 299.03 | 0.8225 | -565.0 | -421.7 | |
| 0.00 | 1.03 | 0.00 | 0.88 | 18.59 | 67.03 | 49.13 | 298.57 | 0.8183 | -719.0 | -644.2 | |
| 0.00 | 1.71 | 0.00 | 1.41 | 18.95 | 64.96 | 47.05 | 299.96 | 0.8013 | 479.0 | 388.6 | |
| 0.00 | 1.37 | 0.00 | 1.13 | 20.36 | 64.34 | 46.44 | 301.87 | 0.8022 | 373.0 | 208.9 | |
| 0.00 | 0.69 | 0.00 | 0.56 | 20.19 | 63.91 | 46.01 | 301.90 | 0.7976 | 399.0 | 316.4 | |
| 0.00 | 1.54 | 0.00 | 1.25 | 19.93 | 63.59 | 45.68 | 301.78 | 0.7935 | 465.0 | 426.5 | |
| 0.00 | 0.60 | 0.00 | 0.49 | 20.27 | 63.71 | 45.81 | 302.09 | 0.7962 | 337.0 | 320.1 | |
| 1.63 | 2.06 | 1.32 | 1.66 | 20.05 | 63.40 | 45.50 | 302.00 | 0.7923 | 557.6 | 465.6 | |
| 0.00 | 0.94 | 0.00 | 0.77 | 20.32 | 63.50 | 45.60 | 302.26 | 0.7946 | 294.0 | 307.9 | |
| 6.43 | 48.87 | 5.13 | 38.91 | 19.89 | 62.76 | 44.86 | 302.17 | 0.7858 | 801.7 | 325.9 | |
| 1.80 | 2.06 | 1.49 | 1.70 | 21.91 | 63.55 | 45.64 | 304.02 | 0.8025 | -470.9 | -456.3 | |
| 7.63 | -14.00 | 6.08 | -14.00 | 20.23 | 62.53 | 44.62 | 302.68 | 0.7854 | 819.6 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.45 | 20.68 | 60.11 | 42.21 | 304.57 | 0.7656 | 684.0 | 600.3 | |
| 0.00 | 1.46 | 0.00 | 1.11 | 20.68 | 59.64 | 41.73 | 304.85 | 0.7612 | 694.0 | 569.4 | |
| 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. | |