| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.02 | 359.27 | 78.43 | 319.42 | -15.23 | 122.61 | 52.22 | 246.84 | 0.8310 | 221.6 | 163.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.36 | 199.79 | 6.95 | 184.05 | -15.40 | 125.11 | 54.72 | 247.59 | 0.8534 | 591.1 | 315.8 | |
| 2.02 | -1.00 | 1.89 | -1.00 | -15.19 | 124.93 | 54.53 | 247.76 | 0.8513 | 554.6 | 999999 | |
| 6.57 | -1.00 | 6.12 | -1.00 | -15.41 | 124.58 | 54.19 | 247.39 | 0.8490 | 700.5 | 999999 | |
| 1.14 | -1.00 | 1.06 | -1.00 | -15.59 | 124.44 | 54.04 | 247.14 | 0.8482 | 788.0 | 999999 | |
| 7.97 | -1.00 | 7.34 | -1.00 | -15.24 | 124.15 | 53.75 | 247.43 | 0.8448 | 906.4 | 999999 | |
| 12.71 | 49.51 | 11.47 | 44.68 | -14.50 | 123.61 | 53.22 | 248.09 | 0.8380 | 763.0 | 225.3 | |
| 2.10 | -1.00 | 1.93 | -1.00 | -15.52 | 123.98 | 53.59 | 247.06 | 0.8442 | 857.6 | 999999 | |
| 13.84 | -1.00 | 12.40 | -1.00 | -14.93 | 123.15 | 52.75 | 247.42 | 0.8351 | 871.3 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.83 | -14.37 | 121.84 | 51.45 | 247.59 | 0.8217 | 782.0 | 601.4 | |
| 1.23 | -1.00 | 1.07 | -1.00 | -14.95 | 121.98 | 51.59 | 246.97 | 0.8248 | 784.6 | 999999 | |
| 0.61 | 3.51 | 0.53 | 3.00 | -14.62 | 121.42 | 51.03 | 247.14 | 0.8186 | 660.7 | 582.2 | |
| 0.00 | 1.31 | 0.00 | 1.14 | -15.17 | 121.61 | 51.22 | 246.57 | 0.8221 | 578.0 | 486.4 | |
| 0.00 | 1.14 | 0.00 | 0.99 | -15.93 | 121.47 | 51.08 | 245.65 | 0.8234 | -287.0 | -242.7 | |
| 6.40 | 9.11 | 5.52 | 7.86 | -15.65 | 121.28 | 50.88 | 245.89 | 0.8207 | -314.9 | -51.0 | |
| 0.70 | 2.45 | 0.59 | 2.06 | -14.35 | 120.61 | 50.21 | 247.13 | 0.8101 | -364.6 | -237.8 | |
| 0.00 | 1.14 | 0.00 | 0.95 | -13.89 | 120.32 | 49.93 | 247.57 | 0.8059 | 343.0 | 299.5 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -14.76 | 120.54 | 50.15 | 246.63 | 0.8109 | 406.0 | 362.4 | |
| 2.89 | 4.91 | 2.41 | 4.08 | -14.32 | 120.21 | 49.82 | 247.02 | 0.8063 | -437.1 | -389.1 | |
| 0.88 | 2.10 | 0.73 | 1.76 | -14.96 | 120.21 | 49.82 | 246.28 | 0.8085 | -272.7 | -143.4 | |
| 0.00 | 1.66 | 0.00 | 1.40 | -15.55 | 120.07 | 49.67 | 245.52 | 0.8092 | -477.0 | -342.6 | |
| 0.00 | 1.23 | 0.00 | 1.01 | -14.78 | 119.68 | 49.29 | 246.26 | 0.8029 | -236.0 | -319.4 | |
| 1.14 | 2.10 | 0.93 | 1.72 | -14.15 | 119.40 | 49.00 | 246.89 | 0.7979 | 575.2 | 494.7 | |
| 0.26 | 6.75 | 0.21 | 5.44 | -13.81 | 119.06 | 48.67 | 247.16 | 0.7935 | -573.7 | -542.1 | |
| 0.00 | 0.53 | 0.00 | 0.43 | -14.98 | 119.36 | 48.97 | 245.90 | 0.8005 | -589.0 | -501.0 | |
| 1.75 | -23.00 | 1.41 | -23.00 | -13.76 | 118.81 | 48.42 | 247.12 | 0.7909 | -776.5 | 999999 | |
| 0.00 | 1.23 | 0.00 | 1.01 | -15.98 | 119.15 | 48.76 | 244.64 | 0.8023 | -406.0 | -258.9 | |
| 1.84 | 3.59 | 1.50 | 2.93 | -15.32 | 118.85 | 48.46 | 245.29 | 0.7969 | -643.6 | -509.2 | |
| 0.00 | 1.23 | 0.00 | 1.01 | -16.06 | 118.94 | 48.55 | 244.46 | 0.8006 | -462.0 | -368.1 | |
| 12.18 | 55.55 | 10.00 | 45.54 | -16.33 | 118.75 | 48.36 | 244.05 | 0.7998 | -718.4 | -266.3 | |
| 0.00 | 1.23 | 0.00 | 0.98 | -15.25 | 118.03 | 47.64 | 245.02 | 0.7888 | -505.0 | -480.1 | |
| 3.15 | -29.00 | 2.56 | -29.00 | -16.44 | 118.13 | 47.74 | 243.65 | 0.7943 | -843.9 | 999999 | |
| 2.28 | 3.51 | 1.81 | 2.79 | -15.18 | 117.65 | 47.25 | 244.92 | 0.7848 | -538.3 | -416.0 | |
| 0.00 | 1.49 | 0.00 | 1.18 | -15.42 | 117.44 | 47.05 | 244.55 | 0.7837 | -617.0 | -479.6 | |
| 0.00 | 1.40 | 0.00 | 1.10 | -15.32 | 117.00 | 46.61 | 244.47 | 0.7790 | -746.0 | -598.6 | |
| 0.00 | 1.14 | 0.00 | 0.89 | -15.67 | 116.61 | 46.21 | 243.87 | 0.7765 | -672.0 | -589.1 | |
| 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. | |