| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.89 | 269.90 | 68.91 | 337.00 | -8.33 | 249.07 | -65.02 | 101.61 | 0.9172 | 294.8 | -111.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 1.11 | -8.33 | 254.38 | -59.71 | 102.67 | 0.8777 | 182.0 | 132.7 | |
| 2.72 | 267.00 | 3.14 | 333.54 | -8.82 | 250.86 | -63.23 | 102.48 | 0.9054 | 580.6 | -109.8 | |
| 4.44 | -2.00 | 5.18 | -2.00 | -8.54 | 250.53 | -63.56 | 102.11 | 0.9074 | 593.1 | 999999 | |
| 0.82 | -2.00 | 0.97 | -2.00 | -8.24 | 249.99 | -64.11 | 101.68 | 0.9109 | 581.8 | 999999 | |
| 3.44 | -2.00 | 4.10 | -2.00 | -7.94 | 249.87 | -64.23 | 101.34 | 0.9114 | 689.5 | 999999 | |
| 14.04 | -2.00 | 17.11 | -2.00 | -8.36 | 249.38 | -64.72 | 101.70 | 0.9153 | 385.1 | 999999 | |
| 14.76 | -2.00 | 18.06 | -2.00 | -7.81 | 249.18 | -64.91 | 101.07 | 0.9160 | 602.3 | 999999 | |
| 1.00 | -2.00 | 1.23 | -2.00 | -7.50 | 248.91 | -65.19 | 100.68 | 0.9175 | 328.1 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.83 | -9.79 | 247.96 | -66.13 | 102.97 | 0.9263 | -405.0 | -459.6 | |
| 2.26 | -2.00 | 2.86 | -2.00 | -7.82 | 248.36 | -65.74 | 100.94 | 0.9215 | 272.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 1.52 | -8.67 | 248.00 | -66.09 | 101.78 | 0.9248 | -370.0 | -320.5 | |
| 5.16 | -2.00 | 6.59 | -2.00 | -8.09 | 248.12 | -65.97 | 101.19 | 0.9234 | 45.9 | 999999 | |
| 2.99 | -2.00 | 3.94 | -2.00 | -9.33 | 247.60 | -66.49 | 102.41 | 0.9281 | -650.8 | 999999 | |
| 4.26 | -2.00 | 5.73 | -2.00 | -9.65 | 247.16 | -66.93 | 102.67 | 0.9312 | -503.0 | 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. | |