| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 193.84 | 930.61 | 99.09 | 476.18 | 8.96 | 100.12 | -6.51 | 26.31 | 0.2499 | 58.9 | 133.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.33 | 74.63 | 4.22 | 37.82 | 8.46 | 105.36 | -1.27 | 5.91 | 0.2133 | -1315.0 | -475.7 | |
| 10.45 | -1.00 | 5.30 | -1.00 | 8.40 | 105.04 | -1.59 | 7.46 | 0.2129 | -1276.5 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.43 | 8.07 | 104.74 | -1.89 | 9.07 | 0.2080 | -714.0 | -542.2 | |
| 3.31 | 9.86 | 1.68 | 5.00 | 8.49 | 104.47 | -2.16 | 9.99 | 0.2159 | -1060.2 | -910.6 | |
| 0.00 | 2.55 | 0.00 | 1.29 | 6.78 | 104.48 | -2.15 | 11.56 | 0.1870 | -992.0 | -782.3 | |
| 0.00 | 2.29 | 0.00 | 1.16 | 6.78 | 104.27 | -2.36 | 12.64 | 0.1878 | -1033.0 | -771.0 | |
| 0.00 | 2.04 | 0.00 | 1.03 | 7.62 | 104.24 | -2.39 | 11.88 | 0.2020 | -1147.0 | -911.3 | |
| 0.00 | 1.87 | 0.00 | 0.95 | 7.80 | 104.03 | -2.60 | 12.69 | 0.2058 | -1000.0 | -688.0 | |
| 0.00 | 0.93 | 0.00 | 0.48 | 9.16 | 103.69 | -2.94 | 12.79 | 0.2298 | -490.0 | -522.6 | |
| 4.67 | 124.52 | 2.38 | 63.42 | 8.89 | 103.63 | -3.00 | 13.31 | 0.2255 | -1072.0 | -529.5 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 9.19 | 103.51 | -3.12 | 13.51 | 0.2310 | -751.0 | -597.5 | |
| 0.00 | 0.93 | 0.00 | 0.47 | 8.59 | 103.22 | -3.41 | 15.43 | 0.2223 | -923.0 | -737.6 | |
| 24.48 | -10.00 | 12.45 | -10.00 | 8.80 | 102.98 | -3.65 | 16.20 | 0.2269 | -1169.6 | 999999 | |
| 0.59 | 2.80 | 0.30 | 1.42 | 7.68 | 102.84 | -3.79 | 18.34 | 0.2094 | -1050.3 | -918.2 | |
| 0.00 | 2.04 | 0.00 | 1.03 | 7.60 | 102.63 | -4.00 | 19.41 | 0.2091 | -919.0 | -829.5 | |
| 1.02 | -10.00 | 0.52 | -10.00 | 9.47 | 102.49 | -4.14 | 17.33 | 0.2401 | -603.9 | 999999 | |
| 20.57 | -10.00 | 10.48 | -10.00 | 9.10 | 102.40 | -4.23 | 18.14 | 0.2347 | -1079.6 | 999999 | |
| 0.00 | 10.03 | 0.00 | 5.09 | 7.96 | 102.27 | -4.36 | 20.41 | 0.2170 | -1139.0 | -928.0 | |
| 0.00 | 3.40 | 0.00 | 1.73 | 8.29 | 102.14 | -4.49 | 20.40 | 0.2231 | -778.0 | -828.5 | |
| 0.00 | 2.55 | 0.00 | 1.30 | 8.65 | 102.14 | -4.49 | 19.86 | 0.2289 | -756.0 | -656.9 | |
| 3.57 | -10.00 | 1.82 | -10.00 | 9.32 | 102.07 | -4.56 | 19.16 | 0.2400 | -921.4 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 8.81 | 101.57 | -5.06 | 21.89 | 0.2348 | 756.0 | 408.4 | |
| 15.64 | 675.15 | 7.96 | 346.31 | 8.45 | 101.45 | -5.18 | 22.95 | 0.2299 | -1107.8 | 350.4 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 9.14 | 101.33 | -5.30 | 22.30 | 0.2417 | -692.0 | -442.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 6.88 | 101.26 | -5.37 | 26.78 | 0.2070 | -812.0 | -710.9 | |
| 0.00 | 1.10 | 0.00 | 0.56 | 7.73 | 100.96 | -5.67 | 26.29 | 0.2223 | 898.0 | 636.5 | |
| 0.00 | 7.56 | 0.00 | 3.87 | 9.36 | 100.81 | -5.82 | 23.85 | 0.2484 | -132.0 | -185.4 | |
| 2.55 | -23.00 | 1.30 | -23.00 | 8.03 | 100.44 | -6.19 | 27.67 | 0.2309 | 1044.1 | 999999 | |
| 0.68 | -23.00 | 0.35 | -23.00 | 8.31 | 100.23 | -6.40 | 27.92 | 0.2367 | 746.0 | 999999 | |
| 3.57 | -23.00 | 1.83 | -23.00 | 9.40 | 99.94 | -6.69 | 26.88 | 0.2553 | 1008.7 | 999999 | |
| 1.27 | -23.00 | 0.65 | -23.00 | 9.07 | 99.47 | -7.16 | 29.13 | 0.2542 | 1021.4 | 999999 | |
| 0.76 | -23.00 | 0.39 | -23.00 | 9.10 | 99.31 | -7.32 | 29.57 | 0.2559 | 1197.3 | 999999 | |
| 12.83 | -23.00 | 6.58 | -23.00 | 9.37 | 99.13 | -7.50 | 29.66 | 0.2615 | 1147.3 | 999999 | |
| 3.06 | -23.00 | 1.57 | -23.00 | 9.89 | 99.06 | -7.57 | 28.93 | 0.2697 | 1021.7 | 999999 | |
| 75.90 | -23.00 | 39.00 | -23.00 | 9.17 | 98.17 | -8.46 | 33.13 | 0.2671 | 1423.0 | 999999 | |
| 0.59 | -23.00 | 0.31 | -23.00 | 9.15 | 97.35 | -9.28 | 35.62 | 0.2745 | 917.9 | 999999 | |
| 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. | |