| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.58 | 224.94 | 19.74 | 115.11 | 16.47 | 354.03 | 4.89 | 340.78 | 0.2494 | -413.9 | -306.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.67 | 358.86 | 9.73 | 325.45 | 0.2866 | -791.0 | -615.8 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 20.11 | 358.80 | 9.66 | 331.73 | 0.3341 | -797.0 | -603.4 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 19.74 | 357.63 | 8.49 | 334.13 | 0.3199 | -922.0 | -726.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 17.16 | 356.69 | 7.56 | 332.65 | 0.2748 | -854.0 | -603.1 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 19.28 | 356.23 | 7.10 | 337.29 | 0.3034 | -703.0 | -540.9 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.13 | 355.92 | 6.78 | 331.33 | 0.2386 | -729.0 | -509.7 | |
| 10.35 | 170.70 | 5.29 | 87.31 | 15.91 | 355.43 | 6.30 | 334.56 | 0.2466 | -1117.7 | -463.2 | |
| 10.35 | -7.00 | 5.29 | -7.00 | 16.23 | 355.12 | 5.99 | 336.20 | 0.2493 | -1287.0 | 999999 | |
| 11.35 | -7.00 | 5.81 | -7.00 | 16.54 | 354.78 | 5.64 | 337.91 | 0.2519 | -1259.2 | 999999 | |
| 5.08 | -7.00 | 2.60 | -7.00 | 16.39 | 354.39 | 5.26 | 339.06 | 0.2470 | -1201.6 | 999999 | |
| 0.36 | -7.00 | 0.19 | -7.00 | 16.73 | 354.37 | 5.24 | 339.65 | 0.2524 | -854.2 | 999999 | |
| 0.00 | 4.09 | 0.00 | 2.08 | 15.61 | 354.15 | 5.01 | 338.74 | 0.2332 | -1066.0 | -878.7 | |
| 0.00 | 1.73 | 0.00 | 0.90 | 20.31 | 353.93 | 4.79 | 345.16 | 0.3072 | -572.0 | -490.0 | |
| 0.00 | 3.36 | 0.00 | 1.70 | 14.83 | 352.39 | 3.26 | 344.86 | 0.2114 | -881.0 | -666.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 20.03 | 352.16 | 3.03 | 350.32 | 0.2964 | -886.0 | -637.0 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 19.04 | 351.98 | 2.85 | 350.29 | 0.2796 | -991.0 | -711.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 19.93 | 351.71 | 2.57 | 351.70 | 0.2936 | -805.0 | -595.6 | |
| 0.00 | 1.73 | 0.00 | 0.90 | 20.54 | 351.55 | 2.42 | 352.48 | 0.3033 | -825.0 | -705.1 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 19.68 | 350.80 | 1.66 | 354.53 | 0.2876 | -872.0 | -799.1 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 19.74 | 350.64 | 1.50 | 355.08 | 0.2884 | -823.0 | -647.4 | |
| 0.00 | 2.45 | 0.00 | 1.25 | 15.77 | 350.13 | 0.99 | 355.65 | 0.2207 | 790.0 | 669.1 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 15.62 | 350.06 | 0.93 | 355.88 | 0.2179 | 743.0 | 644.6 | |
| 0.00 | 3.36 | 0.00 | 1.71 | 15.71 | 349.78 | 0.64 | 357.16 | 0.2192 | 911.0 | 806.5 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.46 | 349.78 | 0.64 | 357.10 | 0.2150 | 894.0 | 676.2 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 15.46 | 349.59 | 0.45 | 357.96 | 0.2148 | 1035.0 | 721.5 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.34 | 349.43 | 0.29 | 358.66 | 0.2126 | 982.0 | 754.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 16.84 | 349.05 | -0.08 | 0.34 | 0.2382 | 680.0 | 579.5 | |
| 1.09 | 1.73 | 0.56 | 0.88 | 16.71 | 348.96 | -0.18 | 0.73 | 0.2361 | 977.5 | 755.8 | |
| 0.00 | 3.27 | 0.00 | 1.67 | 16.56 | 348.76 | -0.37 | 1.53 | 0.2335 | 1269.0 | 1081.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 17.06 | 348.41 | -0.72 | 2.86 | 0.2422 | 836.0 | 707.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 16.71 | 348.03 | -1.10 | 4.48 | 0.2368 | 1034.0 | 882.5 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 16.84 | 347.71 | -1.42 | 5.72 | 0.2394 | 979.0 | 750.9 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 16.46 | 347.56 | -1.58 | 6.53 | 0.2333 | 1019.0 | 768.7 | |
| 0.00 | 2.36 | 0.00 | 1.21 | 17.06 | 347.49 | -1.65 | 6.51 | 0.2435 | 976.0 | 815.0 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 17.28 | 347.01 | -2.13 | 8.25 | 0.2482 | 969.0 | 761.3 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.37 | 345.89 | -3.25 | 12.38 | 0.2532 | 771.0 | 622.8 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 12.88 | 345.80 | -3.34 | 18.49 | 0.1796 | 842.0 | 563.5 | |
| 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. | |