| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.89 | 566.18 | 45.38 | 285.59 | 8.78 | 343.84 | 10.73 | 280.27 | 0.1888 | -678.5 | -314.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.51 | 12.64 | 347.58 | 14.47 | 292.81 | 0.2656 | -975.0 | -784.6 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 13.02 | 347.09 | 13.98 | 294.83 | 0.2605 | -766.0 | -579.0 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 8.93 | 346.70 | 13.59 | 279.18 | 0.2361 | 641.0 | 533.1 | |
| 6.02 | 9.26 | 3.08 | 4.73 | 12.09 | 346.62 | 13.51 | 292.05 | 0.2475 | -1051.6 | -608.4 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.69 | 346.47 | 13.36 | 278.29 | 0.2318 | 945.0 | 793.4 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 13.01 | 346.48 | 13.37 | 295.69 | 0.2511 | -781.0 | -626.2 | |
| 3.60 | 5.30 | 1.83 | 2.71 | 12.90 | 345.87 | 12.76 | 296.28 | 0.2411 | 899.6 | 556.5 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 7.26 | 345.48 | 12.37 | 272.12 | 0.2135 | -901.0 | -689.4 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 8.29 | 345.51 | 12.40 | 276.94 | 0.2150 | 707.0 | 444.5 | |
| 0.00 | 3.06 | 0.00 | 1.55 | 7.15 | 345.26 | 12.14 | 271.58 | 0.2098 | -879.0 | -743.7 | |
| 0.00 | 1.71 | 0.00 | 0.86 | 7.33 | 345.14 | 12.02 | 272.48 | 0.2078 | -781.0 | -525.7 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 12.37 | 345.14 | 12.03 | 295.42 | 0.2264 | -925.0 | -660.1 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 7.94 | 344.87 | 11.76 | 275.53 | 0.2037 | -614.0 | -405.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 13.38 | 344.97 | 11.86 | 299.75 | 0.2312 | 910.0 | 757.9 | |
| 2.34 | 504.38 | 1.18 | 254.36 | 7.74 | 344.68 | 11.57 | 274.56 | 0.2002 | -994.7 | -359.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.53 | 344.36 | 11.25 | 273.59 | 0.1947 | -687.0 | -483.0 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 6.45 | 344.15 | 11.04 | 267.92 | 0.1912 | 730.0 | 565.6 | |
| 0.27 | -15.00 | 0.14 | -15.00 | 8.60 | 344.17 | 11.06 | 279.18 | 0.1931 | -1064.3 | 999999 | |
| 0.00 | 2.70 | 0.00 | 1.36 | 7.51 | 344.05 | 10.94 | 273.53 | 0.1893 | -913.0 | -654.7 | |
| 2.25 | -15.00 | 1.13 | -15.00 | 6.73 | 343.81 | 10.70 | 269.34 | 0.1852 | 963.0 | 999999 | |
| 69.74 | -15.00 | 35.17 | -15.00 | 8.85 | 343.78 | 10.66 | 280.80 | 0.1870 | -1443.6 | 999999 | |
| 0.00 | 2.70 | 0.00 | 1.36 | 7.55 | 343.71 | 10.60 | 273.81 | 0.1835 | -541.0 | -466.6 | |
| 2.88 | -15.00 | 1.45 | -15.00 | 6.52 | 343.59 | 10.48 | 268.15 | 0.1816 | 1055.4 | 999999 | |
| 1.89 | -15.00 | 0.95 | -15.00 | 6.83 | 343.47 | 10.36 | 269.83 | 0.1794 | 930.9 | 999999 | |
| 0.00 | 5.93 | 0.00 | 2.98 | 6.59 | 343.13 | 10.01 | 268.42 | 0.1736 | 1070.0 | 877.8 | |
| 0.00 | 1.71 | 0.00 | 0.86 | 13.22 | 342.93 | 9.82 | 303.66 | 0.2004 | -912.0 | -701.8 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.36 | 342.74 | 9.63 | 272.92 | 0.1669 | 730.0 | 610.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.52 | 342.31 | 9.20 | 274.01 | 0.1596 | 590.0 | 417.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 11.68 | 342.24 | 9.13 | 298.28 | 0.1773 | -915.0 | -779.2 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 11.90 | 342.00 | 8.89 | 300.01 | 0.1754 | -903.0 | -738.3 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 12.85 | 341.28 | 8.17 | 306.83 | 0.1738 | 766.0 | 563.7 | |
| 0.90 | 3.15 | 0.45 | 1.58 | 13.10 | 341.07 | 7.96 | 308.69 | 0.1735 | 1023.5 | 844.0 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 9.46 | 340.62 | 7.51 | 289.04 | 0.1370 | 917.0 | 643.4 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 11.80 | 340.62 | 7.51 | 303.67 | 0.1544 | 834.0 | 669.2 | |
| 0.00 | 1.71 | 0.00 | 0.85 | 9.53 | 340.31 | 7.20 | 290.23 | 0.1323 | 1057.0 | 895.1 | |
| 0.00 | 3.06 | 0.00 | 1.53 | 9.16 | 340.21 | 7.10 | 287.81 | 0.1287 | 895.0 | 751.7 | |
| 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. | |