| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.32 | 26.61 | 0.73 | 14.42 | -8.66 | 9.47 | 23.93 | 262.13 | 0.4069 | 478.3 | 373.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.94 | 0.00 | 1.07 | -8.63 | 12.13 | 26.58 | 262.86 | 0.4478 | 556.0 | 469.1 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -5.40 | 11.80 | 26.26 | 270.15 | 0.4423 | 798.0 | 646.7 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -8.16 | 11.96 | 26.41 | 263.90 | 0.4447 | 706.0 | 551.7 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -8.28 | 11.90 | 26.36 | 263.61 | 0.4439 | 716.0 | 505.7 | |
| 1.32 | 3.17 | 0.73 | 1.74 | -8.34 | 11.39 | 25.85 | 263.43 | 0.4361 | 992.8 | 747.6 | |
| 0.00 | 1.67 | 0.00 | 0.92 | -8.58 | 11.28 | 25.73 | 262.85 | 0.4345 | 933.0 | 790.2 | |
| 0.00 | 2.38 | 0.00 | 1.30 | -8.84 | 10.92 | 25.38 | 262.20 | 0.4293 | 794.0 | 612.9 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -8.66 | 10.74 | 25.20 | 262.57 | 0.4263 | 723.0 | 552.6 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -9.06 | 10.64 | 25.10 | 261.62 | 0.4252 | 757.0 | 589.6 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -5.13 | 9.82 | 24.28 | 271.04 | 0.4113 | 760.0 | 571.4 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -10.47 | 9.31 | 23.76 | 257.86 | 0.4071 | 672.0 | 603.5 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -10.33 | 9.16 | 23.62 | 258.16 | 0.4045 | 778.0 | 548.3 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -9.80 | 8.72 | 23.18 | 259.31 | 0.3964 | 803.0 | 669.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -5.99 | 6.94 | 21.40 | 269.12 | 0.3644 | -602.0 | -427.3 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -7.48 | 6.42 | 20.88 | 264.95 | 0.3563 | -827.0 | -658.0 | |
| 0.00 | 1.85 | 0.00 | 0.98 | -10.88 | 5.61 | 20.07 | 255.07 | 0.3503 | -3.0 | 1.5 | |
| 0.00 | 2.03 | 0.00 | 1.06 | -8.25 | 5.04 | 19.50 | 262.45 | 0.3346 | -702.0 | -670.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -11.78 | 4.12 | 18.58 | 251.47 | 0.3304 | 893.0 | 725.5 | |
| 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. | |