| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.07 | 0.00 | 13.65 | 3.97 | 257.52 | 2.26 | 186.58 | 0.1652 | 479.7 | 349.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.17 | 0.00 | 1.66 | 4.49 | 274.00 | 18.74 | 283.08 | 0.3302 | -981.0 | -734.3 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 4.98 | 272.41 | 17.15 | 285.77 | 0.3065 | -751.0 | -631.4 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 0.09 | 268.11 | 12.85 | 269.37 | 0.2234 | -861.0 | -718.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | -1.65 | 268.08 | 12.82 | 261.61 | 0.2253 | -706.0 | -589.5 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 1.34 | 261.91 | 6.65 | 279.54 | 0.1179 | 794.0 | 523.4 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 5.92 | 260.01 | 4.75 | 320.26 | 0.1295 | 1002.0 | 792.0 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 6.53 | 259.56 | 4.30 | 325.84 | 0.1332 | 785.0 | 671.1 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 10.68 | 257.53 | 2.27 | 347.88 | 0.1864 | 998.0 | 846.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 3.79 | 255.54 | 0.28 | 355.52 | 0.0625 | 899.0 | 668.3 | |
| 0.00 | 3.71 | 0.00 | 1.84 | -0.65 | 254.96 | -0.30 | 160.98 | 0.0164 | 787.0 | 666.0 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 4.19 | 254.11 | -1.15 | 16.23 | 0.0722 | 806.0 | 606.6 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 9.61 | 252.59 | -2.67 | 15.76 | 0.1701 | 913.0 | 674.2 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 8.23 | 251.98 | -3.28 | 22.15 | 0.1508 | 934.0 | 568.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.29 | 250.96 | -4.30 | 40.29 | 0.1161 | 694.0 | 553.4 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 8.75 | 249.11 | -6.16 | 35.57 | 0.1830 | 678.0 | 496.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | -1.35 | 247.14 | -8.12 | 101.01 | 0.1445 | 891.0 | 744.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 1.45 | 243.22 | -12.04 | 84.13 | 0.2106 | 951.0 | 751.0 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 1.55 | 242.72 | -12.54 | 83.94 | 0.2193 | 801.0 | 631.1 | |
| 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. | |