SDO HMI 2011-05-29 00:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.83 | 379.56 | 53.52 | 232.29 | 20.84 | 131.82 | 28.96 | 309.48 | 0.5873 | -174.1 | -126.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.72 | 233.48 | 0.45 | 145.52 | 21.29 | 133.95 | 31.09 | 308.15 | 0.6142 | -615.9 | -352.7 | |
| 0.99 | -1.00 | 0.62 | -1.00 | 21.58 | 133.86 | 31.01 | 308.63 | 0.6155 | -627.5 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 19.48 | 133.32 | 30.47 | 306.12 | 0.5939 | -679.0 | -453.6 | |
| 1.35 | 3.88 | 0.83 | 2.39 | 19.97 | 133.31 | 30.46 | 306.83 | 0.5974 | -716.5 | -589.8 | |
| 6.23 | -1.00 | 3.90 | -1.00 | 21.81 | 133.69 | 30.84 | 309.08 | 0.6153 | -819.4 | 999999 | |
| 27.44 | -1.00 | 17.08 | -1.00 | 21.18 | 133.47 | 30.61 | 308.41 | 0.6081 | -936.5 | 999999 | |
| 7.22 | -1.00 | 4.47 | -1.00 | 20.82 | 133.20 | 30.34 | 308.13 | 0.6024 | -1076.3 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.94 | 19.61 | 132.90 | 30.04 | 306.65 | 0.5900 | 459.0 | 274.3 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 19.93 | 132.97 | 30.11 | 307.07 | 0.5932 | -435.0 | -402.8 | |
| 1.81 | -1.00 | 1.11 | -1.00 | 21.08 | 132.73 | 29.87 | 308.89 | 0.5992 | -858.5 | 999999 | |
| 0.00 | 1.99 | 0.00 | 1.22 | 21.01 | 132.37 | 29.52 | 309.10 | 0.5949 | -912.0 | -729.0 | |
| 0.00 | 1.35 | 0.00 | 0.83 | 21.23 | 132.23 | 29.38 | 309.54 | 0.5952 | -619.0 | -514.9 | |
| 0.00 | 1.53 | 0.00 | 0.94 | 21.50 | 132.11 | 29.25 | 310.02 | 0.5958 | -571.0 | -478.3 | |
| 6.32 | 9.57 | 3.87 | 5.86 | 21.13 | 131.91 | 29.06 | 309.68 | 0.5909 | -920.5 | -627.5 | |
| 2.53 | 3.79 | 1.54 | 2.31 | 20.54 | 131.68 | 28.82 | 309.06 | 0.5835 | -787.1 | -478.3 | |
| 0.00 | 1.71 | 0.00 | 1.05 | 21.06 | 131.49 | 28.63 | 309.97 | 0.5857 | -818.0 | -688.9 | |
| 0.81 | 9.84 | 0.49 | 5.89 | 19.00 | 130.79 | 27.93 | 307.62 | 0.5613 | 820.0 | 686.5 | |
| 0.45 | -17.00 | 0.27 | -17.00 | 19.13 | 130.81 | 27.96 | 307.79 | 0.5626 | 855.4 | 999999 | |
| 11.64 | 15.43 | 6.97 | 9.25 | 19.59 | 130.64 | 27.79 | 308.62 | 0.5643 | 762.1 | 343.4 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 20.93 | 130.87 | 28.01 | 310.35 | 0.5778 | -748.0 | -599.8 | |
| 2.62 | 7.04 | 1.56 | 4.18 | 19.42 | 129.88 | 27.03 | 309.09 | 0.5544 | 836.1 | 605.8 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 18.70 | 129.58 | 26.72 | 308.31 | 0.5449 | 723.0 | 591.5 | |
| 0.00 | 3.43 | 0.00 | 2.03 | 19.22 | 129.34 | 26.49 | 309.33 | 0.5466 | 601.0 | 707.1 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 21.04 | 129.53 | 26.68 | 311.81 | 0.5643 | 576.0 | 456.8 | |
| 0.00 | 1.26 | 0.00 | 0.75 | 19.38 | 129.19 | 26.34 | 309.72 | 0.5462 | 252.0 | 231.6 | |
| 0.00 | 0.72 | 0.00 | 0.43 | 21.14 | 128.82 | 25.97 | 312.66 | 0.5575 | 484.0 | 474.1 | |
| 3.61 | 5.51 | 2.14 | 3.26 | 20.77 | 128.36 | 25.50 | 312.62 | 0.5492 | 764.0 | 670.9 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 20.25 | 128.23 | 25.37 | 312.00 | 0.5431 | 582.0 | 445.1 | |
| 0.00 | 3.07 | 0.00 | 1.81 | 20.48 | 128.16 | 25.31 | 312.40 | 0.5444 | 808.0 | 595.1 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 20.08 | 128.06 | 25.20 | 311.94 | 0.5398 | 676.0 | 573.7 | |
| 0.00 | 2.35 | 0.00 | 1.38 | 20.74 | 127.99 | 25.14 | 312.96 | 0.5450 | 840.0 | 736.4 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 17.39 | 127.07 | 24.21 | 308.85 | 0.5046 | -772.0 | -608.2 | |
| 1.81 | 58.66 | 1.06 | 34.35 | 20.83 | 127.33 | 24.47 | 313.82 | 0.5387 | 764.7 | 494.2 | |
| 1.99 | -33.00 | 1.16 | -33.00 | 20.53 | 127.24 | 24.39 | 313.49 | 0.5350 | 887.0 | 999999 | |
| 0.99 | -33.00 | 0.58 | -33.00 | 20.96 | 127.17 | 24.32 | 314.18 | 0.5383 | 734.0 | 999999 | |
| 5.42 | -33.00 | 3.17 | -33.00 | 20.69 | 126.98 | 24.13 | 314.01 | 0.5338 | 1085.8 | 999999 | |
| 1.17 | 2.98 | 0.67 | 1.70 | 17.48 | 126.42 | 23.57 | 309.73 | 0.4978 | -676.6 | -700.4 | |
| 2.71 | -33.00 | 1.58 | -33.00 | 20.43 | 126.76 | 23.91 | 313.88 | 0.5289 | 902.1 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.72 | 18.03 | 125.90 | 23.05 | 311.20 | 0.4968 | 770.0 | 630.9 | |
| 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. | |