| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.88 | 75.00 | 14.67 | 38.04 | -6.50 | 148.80 | 12.38 | 273.04 | 0.2146 | 528.2 | 139.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.43 | 28.71 | 5.32 | 14.64 | -7.27 | 150.37 | 13.95 | 268.85 | 0.2403 | 1125.3 | 785.6 | |
| 4.05 | -1.00 | 2.06 | -1.00 | -7.16 | 150.12 | 13.70 | 269.33 | 0.2362 | 1204.5 | 999999 | |
| 5.69 | 8.36 | 2.89 | 4.25 | -6.82 | 149.56 | 13.14 | 270.89 | 0.2268 | 1160.7 | 833.2 | |
| 0.52 | 13.71 | 0.26 | 6.95 | -6.59 | 149.18 | 12.77 | 271.99 | 0.2207 | 1098.2 | 893.4 | |
| 3.02 | -4.00 | 1.53 | -4.00 | -6.45 | 148.97 | 12.55 | 272.71 | 0.2171 | 1170.0 | 999999 | |
| 2.84 | -4.00 | 1.44 | -4.00 | -6.31 | 148.66 | 12.24 | 273.49 | 0.2121 | 1183.0 | 999999 | |
| 0.00 | 2.41 | 0.00 | 1.22 | -5.69 | 148.22 | 11.80 | 276.65 | 0.2058 | 659.0 | 500.8 | |
| 0.00 | 1.47 | 0.00 | 0.74 | -4.71 | 146.95 | 10.54 | 282.78 | 0.1878 | -1036.0 | -850.6 | |
| 1.38 | 16.29 | 0.69 | 8.21 | -5.31 | 146.84 | 10.43 | 279.76 | 0.1837 | -1159.7 | -895.0 | |
| 0.95 | -9.00 | 0.48 | -9.00 | -5.64 | 146.85 | 10.43 | 277.99 | 0.1828 | -1085.5 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.65 | -6.33 | 146.25 | 9.84 | 274.51 | 0.1711 | 734.0 | 603.6 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -5.88 | 145.16 | 8.74 | 278.17 | 0.1534 | -951.0 | -712.0 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -5.18 | 144.24 | 7.83 | 284.14 | 0.1405 | -833.0 | -629.4 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -5.85 | 143.29 | 6.87 | 280.84 | 0.1218 | -891.0 | -780.1 | |
| 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. | |