SDO HMI 2011-08-08 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.56 | 265.64 | 46.25 | 137.26 | 19.87 | 241.53 | 9.23 | 327.79 | 0.2847 | -4.7 | 148.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.42 | 0.00 | 2.32 | 19.30 | 246.91 | 14.61 | 313.84 | 0.3315 | -839.0 | -737.0 | |
| 0.00 | 2.44 | 0.00 | 1.28 | 18.90 | 246.64 | 14.34 | 313.41 | 0.3240 | -866.0 | -750.8 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 19.10 | 246.19 | 13.89 | 314.74 | 0.3209 | -1016.0 | -796.9 | |
| 4.06 | 20.86 | 2.12 | 10.86 | 18.82 | 245.91 | 13.61 | 314.67 | 0.3145 | -883.4 | -871.9 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 19.16 | 245.94 | 13.64 | 315.42 | 0.3186 | -905.0 | -651.4 | |
| 0.00 | 2.62 | 0.00 | 1.37 | 19.88 | 245.96 | 13.66 | 316.99 | 0.3271 | -510.0 | -446.8 | |
| 0.00 | 4.97 | 0.00 | 2.60 | 19.57 | 245.80 | 13.50 | 316.62 | 0.3218 | -443.0 | -667.3 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 18.02 | 245.68 | 13.38 | 313.16 | 0.3030 | -727.0 | -600.4 | |
| 11.83 | -4.00 | 6.16 | -4.00 | 18.61 | 245.66 | 13.36 | 314.66 | 0.3092 | -1179.2 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 19.06 | 245.13 | 12.83 | 316.83 | 0.3082 | -789.0 | -608.9 | |
| 1.81 | 8.13 | 0.94 | 4.22 | 18.63 | 244.64 | 12.34 | 316.90 | 0.2977 | -1060.9 | -904.4 | |
| 0.90 | 3.25 | 0.47 | 1.69 | 19.08 | 244.41 | 12.11 | 318.46 | 0.3003 | -871.4 | -783.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 18.89 | 244.36 | 12.06 | 318.13 | 0.2976 | -960.0 | -776.5 | |
| 0.00 | 3.43 | 0.00 | 1.78 | 18.61 | 244.21 | 11.91 | 317.82 | 0.2926 | -993.0 | -830.3 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 18.77 | 244.09 | 11.79 | 318.47 | 0.2932 | -928.0 | -755.6 | |
| 14.36 | 20.77 | 7.41 | 10.72 | 18.44 | 243.58 | 11.28 | 318.90 | 0.2835 | -1179.0 | -869.2 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 18.58 | 243.00 | 10.70 | 320.67 | 0.2789 | -699.0 | -641.6 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 19.48 | 242.99 | 10.69 | 322.76 | 0.2904 | 587.0 | 321.3 | |
| 1.26 | 1.72 | 0.66 | 0.89 | 19.95 | 242.90 | 10.59 | 324.03 | 0.2956 | 725.1 | 575.0 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 20.49 | 242.34 | 10.04 | 326.55 | 0.2975 | 941.0 | 697.9 | |
| 0.00 | 3.07 | 0.00 | 1.59 | 20.68 | 242.19 | 9.89 | 327.31 | 0.2988 | 994.0 | 756.9 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 17.85 | 241.89 | 9.59 | 321.89 | 0.2580 | 892.0 | 696.3 | |
| 6.77 | 9.21 | 3.48 | 4.74 | 18.88 | 241.85 | 9.55 | 324.45 | 0.2711 | -1057.7 | -815.8 | |
| 0.00 | 2.44 | 0.00 | 1.25 | 18.98 | 241.40 | 9.10 | 325.94 | 0.2681 | -881.0 | -801.9 | |
| 1.99 | 3.52 | 1.03 | 1.82 | 20.89 | 241.41 | 9.11 | 329.74 | 0.2948 | 887.5 | 646.6 | |
| 1.72 | 9.48 | 0.88 | 4.87 | 18.86 | 241.16 | 8.86 | 326.36 | 0.2643 | -922.5 | -258.7 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 18.58 | 240.86 | 8.56 | 326.65 | 0.2577 | 968.0 | 819.7 | |
| 3.16 | 30.79 | 1.63 | 15.93 | 20.77 | 240.84 | 8.54 | 331.08 | 0.2885 | 852.3 | 701.8 | |
| 2.44 | -28.00 | 1.26 | -28.00 | 21.15 | 240.50 | 8.20 | 332.70 | 0.2914 | 959.2 | 999999 | |
| 0.72 | -28.00 | 0.37 | -28.00 | 20.81 | 240.42 | 8.12 | 332.35 | 0.2857 | 1295.8 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 22.07 | 240.13 | 7.83 | 335.21 | 0.3022 | 939.0 | 664.0 | |
| 1.44 | 114.21 | 0.74 | 58.81 | 20.53 | 239.91 | 7.61 | 333.35 | 0.2778 | 784.6 | 535.1 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 21.88 | 239.95 | 7.65 | 335.41 | 0.2982 | 733.0 | 636.3 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 19.47 | 239.63 | 7.33 | 332.29 | 0.2600 | 1087.0 | 840.4 | |
| 7.58 | -32.00 | 3.91 | -32.00 | 20.57 | 239.55 | 7.25 | 334.49 | 0.2757 | 1141.7 | 999999 | |
| 16.79 | -32.00 | 8.63 | -32.00 | 20.16 | 239.40 | 7.10 | 334.26 | 0.2685 | 1208.9 | 999999 | |
| 12.73 | -32.00 | 6.56 | -32.00 | 20.82 | 239.17 | 6.87 | 336.06 | 0.2769 | 989.5 | 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. | |