SDO HMI 2011-08-08 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85.42 | 246.67 | 44.19 | 127.68 | 19.87 | 241.59 | 9.84 | 326.11 | 0.2901 | -36.5 | 177.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.79 | 0.00 | 2.00 | 19.32 | 246.93 | 15.18 | 312.85 | 0.3385 | -802.0 | -691.4 | |
| 0.00 | 2.80 | 0.00 | 1.47 | 18.92 | 246.69 | 14.94 | 312.35 | 0.3315 | -985.0 | -718.5 | |
| 0.00 | 2.53 | 0.00 | 1.33 | 19.06 | 246.27 | 14.52 | 313.44 | 0.3279 | -888.0 | -693.6 | |
| 15.80 | 19.23 | 8.25 | 10.05 | 18.70 | 245.81 | 14.06 | 313.46 | 0.3184 | -1117.7 | -887.1 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 18.26 | 245.64 | 13.89 | 312.73 | 0.3118 | -949.0 | -669.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 19.60 | 245.69 | 13.94 | 315.81 | 0.3270 | -801.0 | -616.8 | |
| 0.00 | 1.53 | 0.00 | 0.80 | 19.02 | 245.17 | 13.43 | 315.50 | 0.3146 | -809.0 | -656.9 | |
| 1.44 | 3.07 | 0.75 | 1.60 | 18.71 | 245.05 | 13.30 | 315.02 | 0.3097 | -963.8 | -736.2 | |
| 0.00 | 5.06 | 0.00 | 2.63 | 18.60 | 244.74 | 13.00 | 315.37 | 0.3048 | -1119.0 | -923.0 | |
| 1.81 | 6.59 | 0.94 | 3.43 | 19.07 | 244.49 | 12.74 | 317.05 | 0.3072 | -921.5 | -767.5 | |
| 1.08 | 3.16 | 0.56 | 1.64 | 18.61 | 244.32 | 12.57 | 316.31 | 0.2999 | -907.3 | -752.0 | |
| 0.00 | 3.52 | 0.00 | 1.83 | 18.83 | 244.14 | 12.39 | 317.24 | 0.3005 | -944.0 | -664.5 | |
| 15.44 | 21.31 | 7.99 | 11.03 | 18.43 | 243.65 | 11.90 | 317.40 | 0.2903 | -1168.8 | -845.5 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 18.78 | 243.48 | 11.73 | 318.63 | 0.2925 | -468.0 | -420.9 | |
| 0.00 | 2.53 | 0.00 | 1.31 | 18.48 | 243.10 | 11.35 | 318.81 | 0.2847 | -739.0 | -605.9 | |
| 0.00 | 2.44 | 0.00 | 1.27 | 20.04 | 242.78 | 11.03 | 323.14 | 0.3010 | 826.0 | 707.7 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 18.71 | 242.30 | 10.55 | 321.37 | 0.2790 | -769.0 | -564.1 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 20.59 | 242.29 | 10.54 | 325.46 | 0.3034 | 940.0 | 794.0 | |
| 0.00 | 2.80 | 0.00 | 1.45 | 20.75 | 242.14 | 10.39 | 326.16 | 0.3041 | 824.0 | 758.6 | |
| 5.06 | 8.49 | 2.61 | 4.37 | 18.91 | 241.88 | 10.14 | 322.90 | 0.2773 | -1071.9 | -859.3 | |
| 0.00 | 3.34 | 0.00 | 1.72 | 18.95 | 241.46 | 9.71 | 324.13 | 0.2736 | -895.0 | -750.8 | |
| 1.99 | 9.84 | 1.02 | 5.06 | 18.83 | 241.16 | 9.41 | 324.69 | 0.2691 | -906.9 | 62.2 | |
| 1.44 | 2.98 | 0.75 | 1.55 | 20.98 | 241.29 | 9.55 | 328.75 | 0.2998 | 725.4 | 710.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 18.56 | 240.34 | 8.59 | 326.49 | 0.2576 | 726.0 | 498.0 | |
| 1.99 | 28.17 | 1.03 | 14.60 | 21.18 | 240.45 | 8.70 | 331.37 | 0.2956 | 894.1 | 767.0 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 20.53 | 240.25 | 8.50 | 330.76 | 0.2846 | 820.0 | 612.0 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 22.14 | 240.11 | 8.36 | 333.85 | 0.3069 | 871.0 | 663.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 21.92 | 239.96 | 8.22 | 333.90 | 0.3026 | 889.0 | 666.8 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 19.22 | 239.75 | 8.01 | 329.69 | 0.2617 | 751.0 | 604.1 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 19.41 | 239.57 | 7.82 | 330.64 | 0.2629 | 958.0 | 810.5 | |
| 0.00 | 4.42 | 0.00 | 2.29 | 21.20 | 239.56 | 7.81 | 333.87 | 0.2890 | 855.0 | 686.0 | |
| 11.38 | 90.47 | 5.87 | 46.62 | 20.60 | 239.50 | 7.75 | 333.06 | 0.2797 | 1068.3 | 652.3 | |
| 15.26 | -32.00 | 7.85 | -32.00 | 20.13 | 239.37 | 7.63 | 332.59 | 0.2719 | 1231.5 | 999999 | |
| 0.00 | 2.89 | 0.00 | 1.50 | 21.45 | 239.38 | 7.63 | 334.80 | 0.2915 | -175.0 | -217.6 | |
| 12.73 | -32.00 | 6.57 | -32.00 | 20.86 | 239.15 | 7.40 | 334.51 | 0.2810 | 975.3 | 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. | |