| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.15 | 66.72 | 0.59 | 33.72 | 13.19 | 352.01 | 8.35 | 312.98 | 0.1950 | -235.5 | -282.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.46 | 13.11 | 358.79 | 15.14 | 293.00 | 0.2776 | -719.0 | -546.5 | |
| 0.00 | 1.60 | 0.00 | 0.81 | 11.35 | 357.01 | 13.36 | 288.66 | 0.2401 | -870.0 | -793.9 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 10.28 | 356.27 | 12.62 | 285.00 | 0.2235 | -871.0 | -772.9 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 10.50 | 356.18 | 12.53 | 286.02 | 0.2230 | -819.0 | -629.5 | |
| 0.00 | 2.04 | 0.00 | 1.04 | 13.55 | 356.27 | 12.62 | 298.30 | 0.2423 | -802.0 | -672.1 | |
| 0.00 | 7.45 | 0.00 | 3.78 | 11.20 | 355.90 | 12.25 | 289.41 | 0.2216 | -673.0 | -849.5 | |
| 0.00 | 2.84 | 0.00 | 1.45 | 13.52 | 356.01 | 12.36 | 298.67 | 0.2383 | -839.0 | -750.7 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 11.29 | 355.72 | 12.06 | 290.08 | 0.2192 | -1114.0 | -947.8 | |
| 0.80 | 2.84 | 0.41 | 1.44 | 12.23 | 355.73 | 12.08 | 294.04 | 0.2249 | -1024.1 | -785.3 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 11.39 | 355.56 | 11.91 | 290.71 | 0.2173 | -892.0 | -792.7 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 11.81 | 355.55 | 11.90 | 292.57 | 0.2195 | -855.0 | -673.1 | |
| 0.35 | 4.43 | 0.18 | 2.25 | 12.63 | 355.43 | 11.78 | 296.21 | 0.2230 | -1107.5 | -789.0 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 11.58 | 355.32 | 11.67 | 291.90 | 0.2145 | -712.0 | -625.7 | |
| 0.00 | 4.97 | 0.00 | 2.52 | 12.24 | 355.26 | 11.60 | 294.90 | 0.2177 | -1030.0 | -925.2 | |
| 0.00 | 2.84 | 0.00 | 1.44 | 13.70 | 354.98 | 11.33 | 301.40 | 0.2246 | -894.0 | -771.1 | |
| 0.00 | 1.33 | 0.00 | 0.68 | 13.56 | 354.66 | 11.00 | 301.53 | 0.2187 | -876.0 | -705.3 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 14.23 | 354.47 | 10.82 | 304.58 | 0.2219 | -832.0 | -667.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 14.49 | 353.79 | 10.13 | 307.27 | 0.2150 | -729.0 | -564.1 | |
| 0.00 | 1.60 | 0.00 | 0.81 | 12.50 | 353.54 | 9.89 | 299.52 | 0.1936 | -957.0 | -809.2 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 16.17 | 353.49 | 9.84 | 314.01 | 0.2292 | -818.0 | -644.2 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 13.01 | 353.31 | 9.66 | 302.43 | 0.1946 | -906.0 | -703.3 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 14.66 | 351.40 | 7.75 | 315.30 | 0.1862 | -789.0 | -637.3 | |
| 0.00 | 1.51 | 0.00 | 0.76 | 12.98 | 350.56 | 6.91 | 311.12 | 0.1563 | 881.0 | 687.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 12.35 | 347.51 | 3.86 | 324.12 | 0.1126 | 794.0 | 608.7 | |
| 0.00 | 1.77 | 0.00 | 0.89 | 14.60 | 346.58 | 2.93 | 339.12 | 0.1395 | 710.0 | 621.7 | |
| 0.00 | 1.60 | 0.00 | 0.80 | 13.45 | 346.10 | 2.45 | 339.26 | 0.1179 | 918.0 | 769.7 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 17.31 | 346.00 | 2.34 | 347.53 | 0.1816 | 859.0 | 670.0 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 13.57 | 345.82 | 2.17 | 341.77 | 0.1184 | 1020.0 | 842.1 | |
| 0.00 | 2.22 | 0.00 | 1.11 | 14.42 | 345.62 | 1.96 | 345.31 | 0.1315 | 949.0 | 851.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 14.57 | 345.40 | 1.75 | 347.14 | 0.1332 | 732.0 | 627.9 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 12.03 | 344.98 | 1.33 | 345.11 | 0.0885 | -864.0 | -643.8 | |
| 0.00 | 3.19 | 0.00 | 1.60 | 15.64 | 344.44 | 0.79 | 354.87 | 0.1489 | 1069.0 | 868.2 | |
| 0.00 | 2.13 | 0.00 | 1.06 | 14.73 | 344.31 | 0.66 | 355.18 | 0.1330 | 963.0 | 874.8 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 14.46 | 343.66 | 0.01 | 359.96 | 0.1278 | 632.0 | 576.9 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 13.70 | 343.28 | -0.37 | 3.13 | 0.1148 | 770.0 | 639.3 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 18.76 | 341.37 | -2.28 | 10.59 | 0.2057 | 760.0 | 735.9 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 21.10 | 339.73 | -3.93 | 14.83 | 0.2507 | 703.0 | 573.9 | |
| 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. | |