| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.97 | 31.43 | 3.74 | 20.55 | -17.08 | 99.36 | -34.80 | 123.09 | 0.6501 | -60.6 | 206.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.59 | -16.92 | 104.17 | -29.99 | 126.48 | 0.5970 | -744.0 | -649.8 | |
| 0.00 | 1.21 | 0.00 | 0.76 | -16.35 | 102.42 | -31.74 | 124.22 | 0.6127 | 763.0 | 620.6 | |
| 2.94 | 10.13 | 1.84 | 6.33 | -16.14 | 102.32 | -31.84 | 123.83 | 0.6123 | 990.4 | 773.2 | |
| 0.00 | 1.39 | 0.00 | 0.87 | -16.49 | 102.25 | -31.91 | 124.27 | 0.6156 | 693.0 | 561.9 | |
| 3.03 | 9.09 | 1.90 | 5.71 | -16.12 | 101.95 | -32.21 | 123.52 | 0.6164 | 896.3 | 647.4 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -15.68 | 96.99 | -37.17 | 119.43 | 0.6703 | -597.0 | -514.1 | |
| 0.00 | 1.82 | 0.00 | 1.29 | -18.66 | 94.08 | -40.08 | 121.54 | 0.7181 | -567.0 | -562.9 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -18.10 | 93.70 | -40.46 | 120.62 | 0.7191 | -587.0 | -548.4 | |
| 0.00 | 1.30 | 0.00 | 0.93 | -18.27 | 93.49 | -40.67 | 120.72 | 0.7222 | -511.0 | -345.0 | |
| 0.00 | 1.73 | 0.00 | 1.28 | -19.99 | 92.12 | -42.04 | 122.06 | 0.7450 | -576.0 | -430.5 | |
| 0.00 | 0.78 | 0.00 | 0.58 | -19.49 | 91.72 | -42.44 | 121.25 | 0.7464 | -675.0 | -575.0 | |
| 0.00 | 0.43 | 0.00 | 0.32 | -19.76 | 91.50 | -42.66 | 121.46 | 0.7499 | -583.0 | -541.2 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -16.70 | 91.67 | -42.49 | 117.77 | 0.7335 | -555.0 | -480.0 | |
| 0.00 | 0.69 | 0.00 | 0.56 | -23.99 | 88.91 | -45.25 | 125.02 | 0.7946 | -540.0 | -459.1 | |
| 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. | |