| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.62 | 0.00 | 10.46 | 15.11 | 259.47 | 31.90 | 289.75 | 0.5407 | 269.5 | 188.4 | |
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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 | 0.75 | 13.12 | 271.78 | 44.20 | 282.68 | 0.6983 | -614.0 | -446.1 | |
| 0.00 | 1.90 | 0.00 | 1.22 | 16.00 | 266.46 | 38.88 | 287.98 | 0.6367 | -601.0 | -463.5 | |
| 0.00 | 1.99 | 0.00 | 1.27 | 15.96 | 266.08 | 38.51 | 288.03 | 0.6318 | -625.0 | -401.0 | |
| 0.00 | 0.81 | 0.00 | 0.50 | 15.53 | 262.51 | 34.94 | 288.41 | 0.5837 | -663.0 | -532.1 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 9.86 | 258.94 | 31.36 | 279.11 | 0.5214 | 640.0 | 519.2 | |
| 0.00 | 0.27 | 0.00 | 0.16 | 16.84 | 259.12 | 31.55 | 292.05 | 0.5424 | 371.0 | 454.0 | |
| 0.00 | 2.44 | 0.00 | 1.43 | 17.02 | 258.81 | 31.24 | 292.51 | 0.5389 | 630.0 | 566.0 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 16.80 | 258.74 | 31.17 | 292.16 | 0.5370 | 837.0 | 669.9 | |
| 0.00 | 2.71 | 0.00 | 1.55 | 13.30 | 257.12 | 29.55 | 286.28 | 0.5019 | 484.0 | 430.8 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 16.87 | 257.42 | 29.85 | 292.96 | 0.5193 | 670.0 | 539.5 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 13.27 | 248.80 | 21.22 | 290.74 | 0.3783 | 694.0 | 557.5 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 15.55 | 248.05 | 20.47 | 297.06 | 0.3800 | 746.0 | 539.3 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 15.80 | 247.87 | 20.30 | 297.86 | 0.3792 | 764.0 | 697.7 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 21.79 | 239.95 | 12.38 | 324.03 | 0.3403 | 440.0 | 503.7 | |
| 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. | |