| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.05 | 72.80 | 37.06 | 135.00 | -19.75 | 81.87 | -72.83 | 111.01 | 0.9634 | 114.8 | -5.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.25 | 42.09 | 5.18 | 69.47 | -20.03 | 84.55 | -70.15 | 111.64 | 0.9520 | 603.6 | 53.7 | |
| 0.00 | 1.37 | 0.00 | 2.28 | -20.18 | 83.72 | -70.98 | 111.67 | 0.9562 | 36.0 | 17.9 | |
| 7.96 | -1.00 | 13.02 | -1.00 | -19.76 | 84.07 | -70.63 | 111.28 | 0.9542 | 456.9 | 999999 | |
| 1.20 | 3.76 | 2.25 | 7.09 | -21.31 | 81.75 | -72.94 | 112.57 | 0.9657 | 279.2 | 118.9 | |
| 0.00 | 0.77 | 0.00 | 1.43 | -21.12 | 81.90 | -72.80 | 112.39 | 0.9650 | 209.0 | 221.6 | |
| 1.37 | -1.00 | 2.28 | -1.00 | -19.52 | 83.64 | -71.06 | 110.97 | 0.9561 | -101.1 | 999999 | |
| 0.60 | 1.88 | 1.09 | 3.42 | -20.54 | 82.29 | -72.40 | 111.84 | 0.9629 | -192.0 | -223.3 | |
| 1.11 | -1.00 | 1.88 | -1.00 | -19.06 | 83.24 | -71.46 | 110.44 | 0.9577 | -50.4 | 999999 | |
| 0.00 | 1.37 | 0.00 | 2.66 | -19.68 | 80.92 | -73.78 | 110.79 | 0.9682 | 134.0 | 32.9 | |
| 0.00 | 1.28 | 0.00 | 2.79 | -20.68 | 79.33 | -75.37 | 111.63 | 0.9749 | 57.0 | -11.5 | |
| 0.00 | 0.26 | 0.00 | 0.48 | -18.66 | 81.58 | -73.12 | 109.82 | 0.9649 | -399.0 | -401.0 | |
| 0.00 | 5.65 | 0.00 | 13.88 | -21.07 | 77.76 | -76.93 | 111.86 | 0.9803 | 178.0 | 26.0 | |
| 5.56 | 8.64 | 11.36 | 17.61 | -18.76 | 80.09 | -74.61 | 109.75 | 0.9711 | -320.2 | -360.3 | |
| 0.00 | 0.86 | 0.00 | 1.75 | -18.38 | 79.96 | -74.74 | 109.35 | 0.9715 | -122.0 | -131.9 | |
| 0.00 | 2.22 | 0.00 | 5.11 | -19.46 | 78.36 | -76.34 | 110.29 | 0.9778 | 70.0 | -80.3 | |
| 0.00 | 0.77 | 0.00 | 1.76 | -19.11 | 78.47 | -76.23 | 109.95 | 0.9773 | -156.0 | -138.9 | |
| 0.00 | 1.88 | 0.00 | 5.27 | -17.24 | 75.86 | -78.84 | 107.81 | 0.9850 | -138.0 | -107.6 | |
| 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. | |