SDO HMI 2011-05-29 08:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96.33 | 330.24 | 61.32 | 211.41 | 20.75 | 131.58 | 33.12 | 305.85 | 0.6317 | -193.0 | -113.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.53 | 202.60 | 1.00 | 132.56 | 20.99 | 133.61 | 35.15 | 304.68 | 0.6558 | -576.6 | -304.4 | |
| 4.88 | 7.58 | 3.16 | 4.91 | 20.07 | 133.33 | 34.87 | 303.62 | 0.6470 | -847.7 | -737.0 | |
| 4.15 | -1.00 | 2.74 | -1.00 | 21.98 | 133.60 | 35.14 | 306.00 | 0.6620 | -850.2 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 19.81 | 132.99 | 34.52 | 303.48 | 0.6415 | 113.0 | 106.1 | |
| 27.45 | -1.00 | 17.95 | -1.00 | 21.35 | 133.35 | 34.89 | 305.33 | 0.6553 | -859.7 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.87 | 19.29 | 132.66 | 34.20 | 302.97 | 0.6346 | 711.0 | 504.5 | |
| 7.76 | -1.00 | 5.04 | -1.00 | 20.92 | 132.95 | 34.49 | 305.03 | 0.6482 | -1016.5 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.93 | 20.55 | 132.27 | 33.81 | 305.01 | 0.6383 | -475.0 | -459.0 | |
| 11.56 | -1.00 | 7.45 | -1.00 | 21.17 | 132.23 | 33.77 | 305.88 | 0.6420 | -960.2 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.04 | 20.03 | 131.94 | 33.48 | 304.51 | 0.6313 | -816.0 | -651.9 | |
| 3.16 | 8.31 | 2.02 | 5.32 | 20.62 | 132.05 | 33.59 | 305.25 | 0.6363 | -922.5 | -777.4 | |
| 0.00 | 1.17 | 0.00 | 0.74 | 19.01 | 131.25 | 32.78 | 303.58 | 0.6167 | 552.0 | 363.6 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 19.24 | 131.26 | 32.80 | 303.90 | 0.6184 | 392.0 | 338.7 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 21.20 | 131.69 | 33.23 | 306.32 | 0.6363 | -728.0 | -591.7 | |
| 0.00 | 0.90 | 0.00 | 0.57 | 19.20 | 130.98 | 32.52 | 304.05 | 0.6150 | 458.0 | 405.6 | |
| 0.00 | 1.53 | 0.00 | 0.96 | 18.91 | 130.76 | 32.30 | 303.79 | 0.6105 | 471.0 | 505.2 | |
| 1.08 | 5.60 | 0.68 | 3.48 | 18.94 | 130.58 | 32.12 | 303.97 | 0.6086 | 744.2 | 726.6 | |
| 0.00 | 0.27 | 0.00 | 0.17 | 21.19 | 131.03 | 32.57 | 306.80 | 0.6290 | -652.0 | -688.0 | |
| 1.44 | -17.00 | 0.90 | -17.00 | 18.94 | 130.24 | 31.78 | 304.23 | 0.6046 | 764.2 | 999999 | |
| 6.68 | 16.34 | 4.16 | 10.20 | 19.42 | 130.31 | 31.84 | 304.88 | 0.6087 | 794.5 | 207.8 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 18.74 | 129.90 | 31.43 | 304.20 | 0.5993 | 763.0 | 657.3 | |
| 5.51 | 8.40 | 3.41 | 5.21 | 19.42 | 129.77 | 31.31 | 305.28 | 0.6026 | 767.8 | 397.5 | |
| 0.00 | 1.99 | 0.00 | 1.22 | 18.64 | 129.27 | 30.81 | 304.54 | 0.5914 | 800.0 | 587.9 | |
| 3.34 | 3.52 | 2.06 | 2.17 | 19.32 | 129.26 | 30.80 | 305.54 | 0.5961 | 759.4 | 569.5 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 21.11 | 128.79 | 30.32 | 308.48 | 0.6039 | 682.0 | 498.5 | |
| 1.63 | 3.52 | 1.00 | 2.17 | 20.94 | 128.30 | 29.83 | 308.66 | 0.5973 | 642.9 | 410.4 | |
| 0.00 | 1.35 | 0.00 | 0.83 | 20.61 | 127.93 | 29.46 | 308.52 | 0.5906 | 669.0 | 505.7 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 20.15 | 127.83 | 29.37 | 307.94 | 0.5860 | 746.0 | 614.7 | |
| 0.00 | 1.99 | 0.00 | 1.21 | 20.24 | 127.66 | 29.20 | 308.23 | 0.5849 | 944.0 | 775.4 | |
| 0.00 | 1.63 | 0.00 | 0.99 | 20.54 | 127.46 | 29.00 | 308.82 | 0.5850 | 798.0 | 707.5 | |
| 1.35 | 40.00 | 0.82 | 24.30 | 20.53 | 127.20 | 28.74 | 309.05 | 0.5821 | 924.3 | 572.7 | |
| 2.17 | -31.00 | 1.32 | -31.00 | 20.86 | 127.24 | 28.77 | 309.49 | 0.5850 | 781.8 | 999999 | |
| 4.24 | 9.93 | 2.52 | 5.89 | 17.68 | 126.48 | 28.02 | 305.44 | 0.5515 | -957.6 | -553.8 | |
| 8.40 | -31.00 | 5.09 | -31.00 | 20.56 | 126.88 | 28.41 | 309.39 | 0.5787 | 979.2 | 999999 | |
| 0.00 | 2.98 | 0.00 | 1.76 | 18.03 | 126.00 | 27.54 | 306.43 | 0.5485 | 735.0 | 565.5 | |
| 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. | |