| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.74 | 0.00 | 11.85 | -13.94 | 205.46 | 37.33 | 252.08 | 0.6208 | -638.9 | -612.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.93 | 0.00 | 0.60 | -13.59 | 206.77 | 38.64 | 253.03 | 0.6369 | -581.0 | -453.5 | |
| 0.00 | 0.85 | 0.00 | 0.55 | -13.89 | 206.83 | 38.70 | 252.59 | 0.6384 | -614.0 | -457.2 | |
| 0.00 | 0.68 | 0.00 | 0.44 | -14.02 | 206.70 | 38.57 | 252.35 | 0.6371 | -599.0 | -548.0 | |
| 0.00 | 0.76 | 0.00 | 0.49 | -13.64 | 206.47 | 38.34 | 252.88 | 0.6331 | -519.0 | -551.2 | |
| 0.00 | 0.59 | 0.00 | 0.38 | -15.64 | 206.77 | 38.64 | 249.89 | 0.6427 | -494.0 | -411.9 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -13.69 | 205.90 | 37.77 | 252.62 | 0.6258 | -735.0 | -581.5 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -13.62 | 205.43 | 37.29 | 252.59 | 0.6195 | -728.0 | -644.3 | |
| 0.00 | 3.48 | 0.00 | 2.19 | -13.89 | 205.29 | 37.15 | 252.10 | 0.6184 | -629.0 | -662.7 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -13.66 | 205.13 | 37.00 | 252.43 | 0.6157 | -694.0 | -677.9 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -13.34 | 204.84 | 36.71 | 252.85 | 0.6110 | -659.0 | -600.1 | |
| 0.00 | 1.02 | 0.00 | 0.64 | -14.32 | 205.03 | 36.89 | 251.33 | 0.6163 | -615.0 | -422.5 | |
| 0.00 | 1.78 | 0.00 | 1.12 | -13.88 | 204.90 | 36.77 | 252.00 | 0.6133 | -950.0 | -792.5 | |
| 0.00 | 2.97 | 0.00 | 1.86 | -13.55 | 204.84 | 36.71 | 252.51 | 0.6116 | -798.0 | -737.5 | |
| 0.00 | 1.02 | 0.00 | 0.64 | -16.14 | 204.86 | 36.73 | 248.40 | 0.6201 | -329.0 | -370.8 | |
| 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. | |