| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.95 | 268.49 | 87.12 | 407.77 | -13.16 | 107.47 | -71.76 | 101.50 | 0.9442 | -17.6 | -231.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.20 | -11.95 | 129.57 | -49.66 | 99.63 | 0.7587 | 491.0 | 509.0 | |
| 0.00 | 0.95 | 0.00 | 0.76 | -13.09 | 126.72 | -52.51 | 101.05 | 0.7897 | 604.0 | 429.5 | |
| 0.00 | 2.41 | 0.00 | 2.00 | -15.20 | 125.33 | -53.90 | 103.65 | 0.8046 | 387.0 | 379.4 | |
| 0.00 | 1.38 | 0.00 | 1.14 | -14.95 | 125.32 | -53.91 | 103.34 | 0.8046 | 510.0 | 419.1 | |
| 0.00 | 3.10 | 0.00 | 2.53 | -11.21 | 126.00 | -53.23 | 98.67 | 0.7971 | 525.0 | 402.1 | |
| 0.00 | 1.55 | 0.00 | 1.25 | -5.43 | 126.93 | -52.30 | 91.32 | 0.7902 | 324.0 | 249.4 | |
| 0.00 | 0.60 | 0.00 | 0.71 | -16.01 | 113.17 | -66.06 | 104.38 | 0.9087 | 177.0 | 198.9 | |
| 0.00 | 3.88 | 0.00 | 4.89 | -12.54 | 111.39 | -67.83 | 100.63 | 0.9215 | -556.0 | -490.4 | |
| 0.78 | 2.58 | 0.99 | 3.30 | -12.15 | 111.12 | -68.11 | 100.21 | 0.9234 | 176.4 | 108.1 | |
| 0.00 | 0.78 | 0.00 | 1.05 | -14.32 | 109.60 | -69.62 | 102.62 | 0.9324 | 22.0 | 41.6 | |
| 0.00 | 1.03 | 0.00 | 1.41 | -12.20 | 109.46 | -69.77 | 100.35 | 0.9339 | -87.0 | -40.2 | |
| 0.00 | 1.03 | 0.00 | 1.47 | -13.64 | 108.52 | -70.71 | 101.95 | 0.9390 | -466.0 | -476.2 | |
| 0.00 | 0.52 | 0.00 | 0.72 | -13.13 | 108.87 | -70.36 | 101.39 | 0.9371 | -545.0 | -500.2 | |
| 19.64 | 245.32 | 29.58 | 381.28 | -13.93 | 107.34 | -71.89 | 102.31 | 0.9457 | -548.6 | -244.4 | |
| 1.21 | -14.00 | 1.90 | -14.00 | -14.58 | 106.30 | -72.93 | 103.04 | 0.9511 | -319.1 | 999999 | |
| 0.00 | 3.10 | 0.00 | 5.06 | -15.05 | 105.66 | -73.57 | 103.58 | 0.9542 | -441.0 | -383.1 | |
| 35.32 | -14.00 | 54.65 | -14.00 | -12.71 | 106.84 | -72.39 | 101.05 | 0.9488 | 255.2 | 999999 | |
| 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. | |