SDO HMI 2011-05-29 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 109.96 | 379.90 | 68.71 | 238.59 | 20.74 | 131.65 | 31.55 | 307.08 | 0.6145 | -232.1 | -98.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.96 | 14.90 | 3.79 | 9.45 | 20.04 | 133.32 | 33.22 | 304.75 | 0.6286 | -809.6 | -258.2 | |
| 5.42 | 210.19 | 3.50 | 135.03 | 21.92 | 133.64 | 33.54 | 307.07 | 0.6446 | -839.2 | -308.1 | |
| 32.41 | -2.00 | 20.79 | -2.00 | 21.25 | 133.39 | 33.28 | 306.37 | 0.6374 | -873.3 | 999999 | |
| 3.61 | -2.00 | 2.31 | -2.00 | 20.92 | 133.19 | 33.08 | 306.06 | 0.6330 | -1022.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 19.39 | 132.59 | 32.49 | 304.36 | 0.6159 | 663.0 | 487.0 | |
| 3.07 | -2.00 | 1.95 | -2.00 | 20.86 | 132.90 | 32.79 | 306.18 | 0.6293 | -1082.8 | 999999 | |
| 13.36 | 15.44 | 8.45 | 9.76 | 21.14 | 132.16 | 32.05 | 307.15 | 0.6232 | -913.1 | -679.5 | |
| 4.79 | 5.60 | 3.01 | 3.52 | 20.52 | 131.97 | 31.87 | 306.43 | 0.6167 | -900.8 | -727.1 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 19.34 | 131.33 | 31.22 | 305.26 | 0.6012 | 270.0 | 261.2 | |
| 0.00 | 2.44 | 0.00 | 1.53 | 21.10 | 131.50 | 31.39 | 307.62 | 0.6157 | -717.0 | -609.8 | |
| 0.00 | 2.62 | 0.00 | 1.61 | 18.98 | 130.91 | 30.81 | 305.06 | 0.5939 | 703.0 | 612.7 | |
| 0.00 | 1.26 | 0.00 | 0.79 | 20.87 | 131.21 | 31.11 | 307.52 | 0.6109 | -831.0 | -615.8 | |
| 0.72 | 6.77 | 0.44 | 4.15 | 18.94 | 130.68 | 30.58 | 305.20 | 0.5910 | 751.5 | 736.2 | |
| 0.00 | 1.72 | 0.00 | 1.07 | 21.10 | 130.89 | 30.78 | 308.11 | 0.6090 | -774.0 | -521.1 | |
| 7.76 | 30.79 | 4.76 | 18.87 | 19.46 | 130.49 | 30.38 | 306.11 | 0.5925 | 859.0 | 153.5 | |
| 1.53 | -15.00 | 0.94 | -15.00 | 19.68 | 130.16 | 30.06 | 306.71 | 0.5904 | 534.4 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 18.81 | 129.98 | 29.88 | 305.57 | 0.5819 | 757.0 | 675.0 | |
| 0.00 | 0.90 | 0.00 | 0.57 | 22.21 | 130.62 | 30.51 | 309.86 | 0.6146 | -656.0 | -516.3 | |
| 5.51 | -15.00 | 3.36 | -15.00 | 19.39 | 129.84 | 29.74 | 306.55 | 0.5846 | 804.0 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.76 | 18.64 | 129.36 | 29.26 | 305.85 | 0.5735 | 830.0 | 638.5 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 14.39 | 128.66 | 28.56 | 299.69 | 0.5351 | -728.0 | -544.9 | |
| 2.80 | 3.34 | 1.70 | 2.02 | 19.29 | 129.30 | 29.20 | 306.86 | 0.5776 | 829.4 | 758.2 | |
| 0.00 | 1.44 | 0.00 | 0.88 | 21.01 | 128.80 | 28.70 | 309.79 | 0.5855 | 582.0 | 461.3 | |
| 1.99 | 3.97 | 1.20 | 2.41 | 20.87 | 128.29 | 28.19 | 310.07 | 0.5789 | 726.7 | 489.3 | |
| 0.00 | 4.06 | 0.00 | 2.44 | 20.05 | 127.94 | 27.84 | 309.21 | 0.5683 | 702.0 | 553.4 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 20.58 | 127.94 | 27.83 | 309.98 | 0.5725 | 824.0 | 641.2 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 16.57 | 127.23 | 27.13 | 304.52 | 0.5325 | -755.0 | -569.6 | |
| 0.00 | 3.25 | 0.00 | 1.97 | 20.87 | 127.96 | 27.85 | 310.38 | 0.5752 | 677.0 | 576.9 | |
| 0.00 | 2.08 | 0.00 | 1.25 | 20.25 | 127.65 | 27.55 | 309.77 | 0.5666 | 856.0 | 716.7 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 17.30 | 126.99 | 26.88 | 305.93 | 0.5352 | -767.0 | -565.0 | |
| 2.17 | 51.28 | 1.30 | 30.70 | 20.57 | 127.24 | 27.13 | 310.64 | 0.5648 | 899.6 | 504.0 | |
| 5.69 | -31.00 | 3.42 | -31.00 | 20.90 | 127.30 | 27.20 | 311.04 | 0.5683 | 724.8 | 999999 | |
| 4.60 | -31.00 | 2.75 | -31.00 | 20.63 | 126.96 | 26.85 | 311.00 | 0.5623 | 1054.3 | 999999 | |
| 4.33 | 5.51 | 2.53 | 3.22 | 17.68 | 126.44 | 26.34 | 307.06 | 0.5317 | -844.8 | -724.9 | |
| 3.07 | -31.00 | 1.83 | -31.00 | 20.40 | 126.73 | 26.63 | 310.89 | 0.5578 | 988.4 | 999999 | |
| 1.17 | 4.06 | 0.68 | 2.37 | 18.03 | 126.00 | 25.89 | 308.05 | 0.5294 | 619.5 | 206.6 | |
| 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. | |