| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.43 | 307.09 | 34.45 | 154.42 | 14.01 | 56.57 | 5.82 | 323.83 | 0.1703 | -238.1 | -190.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 0.77 | 9.62 | 60.61 | 9.86 | 287.11 | 0.1774 | -959.0 | -833.4 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 9.51 | 60.29 | 9.54 | 286.95 | 0.1717 | -973.0 | -828.2 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 11.58 | 60.20 | 9.45 | 298.08 | 0.1832 | -936.0 | -774.3 | |
| 18.10 | 29.62 | 9.16 | 14.99 | 14.02 | 60.14 | 9.39 | 309.00 | 0.2046 | -1156.6 | -513.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 11.53 | 59.64 | 8.89 | 299.26 | 0.1743 | -998.0 | -835.2 | |
| 0.00 | 2.07 | 0.00 | 1.04 | 12.05 | 59.37 | 8.62 | 302.61 | 0.1749 | -836.0 | -711.5 | |
| 0.00 | 3.15 | 0.00 | 1.59 | 12.36 | 59.26 | 8.51 | 304.44 | 0.1760 | -953.0 | -800.7 | |
| 0.00 | 2.70 | 0.00 | 1.36 | 11.90 | 59.21 | 8.46 | 302.34 | 0.1712 | -819.0 | -808.9 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 12.97 | 59.22 | 8.47 | 307.40 | 0.1814 | -703.0 | -507.0 | |
| 0.00 | 1.80 | 0.00 | 0.90 | 10.53 | 58.98 | 8.23 | 295.57 | 0.1568 | -1075.0 | -827.8 | |
| 0.00 | 6.12 | 0.00 | 3.08 | 12.18 | 59.00 | 8.25 | 304.37 | 0.1707 | -1075.0 | -893.6 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 14.58 | 57.98 | 7.23 | 318.42 | 0.1843 | -724.0 | -535.3 | |
| 0.00 | 1.89 | 0.00 | 0.96 | 16.54 | 58.05 | 7.30 | 324.55 | 0.2110 | -480.0 | -502.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 16.33 | 58.01 | 7.26 | 324.08 | 0.2077 | -928.0 | -795.1 | |
| 0.63 | 7.11 | 0.32 | 3.61 | 16.73 | 58.00 | 7.25 | 325.28 | 0.2130 | -974.6 | -792.0 | |
| 0.99 | 145.87 | 0.50 | 73.30 | 14.06 | 57.84 | 7.09 | 316.99 | 0.1762 | -824.6 | -477.8 | |
| 37.28 | -16.00 | 18.74 | -16.00 | 13.76 | 57.70 | 6.95 | 316.29 | 0.1709 | -1248.3 | 999999 | |
| 0.36 | 2.16 | 0.18 | 1.09 | 16.39 | 57.76 | 7.01 | 325.21 | 0.2061 | -1155.0 | -1016.8 | |
| 1.71 | 7.38 | 0.86 | 3.72 | 14.67 | 57.67 | 6.92 | 320.00 | 0.1821 | -934.7 | -877.2 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 14.74 | 57.23 | 6.48 | 322.06 | 0.1782 | -698.0 | -577.0 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 16.52 | 57.16 | 6.41 | 327.91 | 0.2023 | -358.0 | -288.6 | |
| 0.00 | 1.53 | 0.00 | 0.77 | 14.25 | 57.02 | 6.27 | 321.14 | 0.1696 | -537.0 | -480.8 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 13.25 | 56.49 | 5.74 | 319.49 | 0.1506 | 564.0 | 395.6 | |
| 0.00 | 8.10 | 0.00 | 4.06 | 13.07 | 56.15 | 5.39 | 320.43 | 0.1444 | 848.0 | 763.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 12.83 | 56.14 | 5.39 | 319.33 | 0.1412 | 828.0 | 573.2 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 12.56 | 56.04 | 5.29 | 318.53 | 0.1365 | 829.0 | 601.6 | |
| 0.99 | 10.90 | 0.50 | 5.46 | 13.50 | 55.94 | 5.19 | 323.38 | 0.1480 | 918.4 | 163.0 | |
| 0.99 | 2.97 | 0.50 | 1.49 | 13.05 | 55.36 | 4.61 | 324.62 | 0.1359 | 974.5 | 760.2 | |
| 0.45 | 1.44 | 0.22 | 0.72 | 12.78 | 55.33 | 4.58 | 323.60 | 0.1317 | -782.2 | -646.5 | |
| 0.81 | 1.62 | 0.40 | 0.81 | 12.85 | 54.58 | 3.83 | 328.59 | 0.1255 | -928.4 | -872.4 | |
| 0.00 | 2.07 | 0.00 | 1.03 | 13.04 | 53.83 | 3.08 | 334.49 | 0.1222 | 961.0 | 672.4 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 15.34 | 52.45 | 1.70 | 349.17 | 0.1530 | 718.0 | 520.5 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 14.51 | 52.29 | 1.54 | 349.14 | 0.1384 | 924.0 | 710.9 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 14.70 | 52.01 | 1.26 | 351.30 | 0.1407 | 866.0 | 722.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 15.49 | 51.54 | 0.79 | 355.02 | 0.1535 | 735.0 | 643.0 | |
| 0.00 | 2.07 | 0.00 | 1.04 | 15.16 | 51.32 | 0.57 | 356.26 | 0.1474 | 928.0 | 662.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 17.77 | 51.33 | 0.58 | 357.12 | 0.1925 | 860.0 | 714.1 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 13.72 | 51.09 | 0.34 | 357.26 | 0.1222 | 947.0 | 747.1 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 14.61 | 51.10 | 0.35 | 357.56 | 0.1376 | 971.0 | 793.9 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 16.02 | 51.10 | 0.35 | 357.92 | 0.1621 | 856.0 | 688.0 | |
| 1.44 | 7.20 | 0.72 | 3.61 | 15.13 | 51.00 | 0.25 | 358.33 | 0.1466 | 1187.4 | 949.5 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 14.06 | 50.78 | 0.03 | 359.76 | 0.1279 | 941.0 | 701.1 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 14.64 | 50.47 | -0.28 | 1.98 | 0.1381 | 933.0 | 756.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 15.31 | 50.37 | -0.38 | 2.43 | 0.1499 | 775.0 | 610.9 | |
| 0.00 | 1.71 | 0.00 | 0.86 | 15.99 | 50.31 | -0.44 | 2.62 | 0.1616 | 944.0 | 855.3 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 13.29 | 50.13 | -0.62 | 5.31 | 0.1151 | 885.0 | 720.5 | |
| 4.68 | 10.81 | 2.35 | 5.42 | 15.87 | 50.03 | -0.72 | 4.38 | 0.1598 | 1152.3 | 800.6 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 14.58 | 50.03 | -0.72 | 5.10 | 0.1375 | 990.0 | 872.9 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 17.71 | 49.86 | -0.89 | 4.43 | 0.1918 | 561.0 | 440.0 | |
| 0.00 | 4.50 | 0.00 | 2.24 | 13.08 | 49.41 | -1.34 | 11.66 | 0.1133 | 1102.0 | 862.7 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 15.59 | 49.30 | -1.45 | 8.98 | 0.1565 | 841.0 | 708.4 | |
| 0.00 | 1.71 | 0.00 | 0.86 | 16.45 | 49.17 | -1.58 | 8.90 | 0.1715 | 868.0 | 677.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 14.94 | 49.18 | -1.57 | 10.50 | 0.1458 | 792.0 | 665.0 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 16.29 | 49.02 | -1.74 | 9.93 | 0.1693 | 983.0 | 801.2 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 13.63 | 48.85 | -1.90 | 15.07 | 0.1248 | 889.0 | 728.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 17.68 | 48.78 | -1.97 | 9.79 | 0.1935 | 922.0 | 695.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.65 | 48.43 | -2.32 | 11.51 | 0.1941 | 696.0 | 514.4 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 17.74 | 47.63 | -3.12 | 15.18 | 0.1987 | 775.0 | 512.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 17.06 | 47.26 | -3.49 | 17.97 | 0.1894 | 788.0 | 595.2 | |
| 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. | |