| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.82 | 184.85 | 29.26 | 149.13 | 23.56 | 302.34 | 51.42 | 294.60 | 0.7884 | -122.5 | -63.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.86 | 130.02 | 20.15 | 109.91 | 22.79 | 304.88 | 53.96 | 292.98 | 0.8120 | -954.1 | -209.7 | |
| 0.00 | 1.16 | 0.00 | 0.95 | 22.86 | 303.54 | 52.62 | 293.28 | 0.7994 | -525.0 | -462.0 | |
| 0.00 | 1.34 | 0.00 | 1.09 | 23.01 | 303.30 | 52.38 | 293.51 | 0.7973 | -567.0 | -536.7 | |
| 0.00 | 1.16 | 0.00 | 0.91 | 24.73 | 301.07 | 50.15 | 296.13 | 0.7789 | -275.0 | -287.5 | |
| 0.00 | 1.07 | 0.00 | 0.83 | 25.66 | 300.13 | 49.21 | 297.53 | 0.7719 | -522.0 | -517.8 | |
| 0.00 | 1.16 | 0.00 | 0.90 | 25.94 | 299.98 | 49.06 | 297.92 | 0.7710 | -599.0 | -512.2 | |
| 0.00 | 2.68 | 0.00 | 1.93 | 25.41 | 296.00 | 45.07 | 298.39 | 0.7292 | 620.0 | 451.7 | |
| 0.00 | 1.61 | 0.00 | 1.15 | 24.75 | 295.36 | 44.44 | 297.71 | 0.7205 | 619.0 | 432.8 | |
| 0.00 | 1.07 | 0.00 | 0.77 | 25.45 | 295.58 | 44.66 | 298.57 | 0.7251 | 600.0 | 519.0 | |
| 0.00 | 0.89 | 0.00 | 0.64 | 25.59 | 295.42 | 44.50 | 298.81 | 0.7237 | 482.0 | 443.9 | |
| 1.97 | 2.23 | 1.40 | 1.59 | 25.52 | 295.10 | 44.18 | 298.83 | 0.7202 | 662.3 | 519.0 | |
| 0.00 | 0.45 | 0.00 | 0.32 | 25.85 | 294.98 | 44.06 | 299.32 | 0.7200 | 484.0 | 421.0 | |
| 1.61 | 10.72 | 1.15 | 7.67 | 26.53 | 295.02 | 44.10 | 300.21 | 0.7228 | 804.2 | 455.2 | |
| 0.00 | 1.16 | 0.00 | 0.82 | 25.75 | 294.60 | 43.68 | 299.31 | 0.7157 | 609.0 | 517.5 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 25.41 | 294.40 | 43.48 | 298.93 | 0.7124 | 472.0 | 457.1 | |
| 1.52 | -13.00 | 1.08 | -13.00 | 26.67 | 294.90 | 43.98 | 300.44 | 0.7220 | 575.6 | 999999 | |
| 2.77 | 3.57 | 1.95 | 2.52 | 25.87 | 294.33 | 43.41 | 299.57 | 0.7133 | 719.4 | 527.8 | |
| 0.00 | 3.93 | 0.00 | 2.75 | 25.47 | 294.10 | 43.18 | 299.11 | 0.7094 | 727.0 | 693.2 | |
| 0.00 | 2.50 | 0.00 | 1.75 | 25.79 | 293.83 | 42.91 | 299.63 | 0.7076 | 789.0 | 685.1 | |
| 0.00 | 2.77 | 0.00 | 1.95 | 26.35 | 294.04 | 43.12 | 300.32 | 0.7119 | 452.0 | 471.9 | |
| 3.84 | 5.54 | 2.66 | 3.84 | 25.20 | 293.48 | 42.56 | 298.96 | 0.7018 | 776.8 | 455.4 | |
| 0.00 | 1.07 | 0.00 | 0.75 | 26.41 | 293.75 | 42.83 | 300.51 | 0.7090 | 518.0 | 488.9 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 25.75 | 293.45 | 42.53 | 299.73 | 0.7034 | 448.0 | 441.1 | |
| 0.00 | 1.97 | 0.00 | 1.38 | 26.93 | 293.76 | 42.84 | 301.21 | 0.7111 | 730.0 | 523.1 | |
| 0.00 | 0.89 | 0.00 | 0.62 | 26.60 | 293.46 | 42.54 | 300.87 | 0.7067 | 686.0 | 588.8 | |
| 1.25 | 2.14 | 0.87 | 1.49 | 26.35 | 293.22 | 42.29 | 300.64 | 0.7032 | 758.5 | 685.4 | |
| 0.00 | 2.32 | 0.00 | 1.60 | 25.64 | 292.85 | 41.93 | 299.80 | 0.6966 | 838.0 | 635.7 | |
| 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. | |