SDO HMI 2014-04-18 20:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.81 | 848.89 | 43.45 | 441.26 | -16.29 | 222.16 | 13.61 | 228.19 | 0.3015 | 357.3 | 175.1 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.68 | 0.00 | 0.92 | -17.66 | 230.73 | 22.17 | 238.53 | 0.4233 | 817.0 | 647.2 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -17.84 | 230.72 | 22.16 | 238.13 | 0.4245 | 789.0 | 688.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -16.22 | 229.27 | 20.71 | 240.16 | 0.3932 | -578.0 | -460.1 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -10.92 | 227.37 | 18.81 | 252.09 | 0.3342 | 845.0 | 696.7 | |
| 37.91 | 296.08 | 20.17 | 157.35 | -16.38 | 227.22 | 18.66 | 237.40 | 0.3660 | 1343.9 | 396.1 | |
| 0.00 | 1.59 | 0.00 | 0.84 | -13.72 | 226.95 | 18.39 | 243.83 | 0.3431 | -916.0 | -743.6 | |
| 11.69 | -5.00 | 6.20 | -5.00 | -15.86 | 227.07 | 18.51 | 238.47 | 0.3599 | 1365.3 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.02 | -11.26 | 225.87 | 17.31 | 249.77 | 0.3124 | 752.0 | 733.8 | |
| 0.00 | 3.19 | 0.00 | 1.67 | -14.98 | 225.58 | 17.03 | 238.76 | 0.3323 | 1004.0 | 714.1 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -11.46 | 225.24 | 16.68 | 248.53 | 0.3037 | 835.0 | 647.3 | |
| 0.35 | 1.59 | 0.19 | 0.83 | -13.89 | 225.34 | 16.78 | 241.42 | 0.3206 | -879.2 | -677.2 | |
| 0.00 | 3.10 | 0.00 | 1.61 | -11.74 | 225.16 | 16.60 | 247.58 | 0.3040 | 787.0 | 727.9 | |
| 0.00 | 1.51 | 0.00 | 0.79 | -13.77 | 225.20 | 16.64 | 241.57 | 0.3177 | -680.0 | -630.4 | |
| 0.00 | 1.51 | 0.00 | 0.78 | -11.47 | 223.61 | 15.06 | 246.61 | 0.2786 | 894.0 | 689.0 | |
| 0.00 | 1.59 | 0.00 | 0.83 | -14.28 | 223.11 | 14.55 | 236.95 | 0.2918 | 887.0 | 676.6 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -15.66 | 222.49 | 13.94 | 231.87 | 0.2961 | 694.0 | 510.9 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -14.39 | 222.15 | 13.60 | 234.91 | 0.2796 | 808.0 | 645.0 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -17.39 | 221.84 | 13.28 | 226.04 | 0.3060 | 702.0 | 483.4 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -16.12 | 221.27 | 12.71 | 228.15 | 0.2851 | 796.0 | 555.0 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -14.41 | 220.98 | 12.42 | 232.48 | 0.2638 | 925.0 | 771.4 | |
| 0.80 | 37.55 | 0.41 | 19.24 | -13.92 | 220.89 | 12.33 | 233.82 | 0.2579 | 1052.7 | 686.5 | |
| 0.62 | 5.58 | 0.32 | 2.88 | -16.37 | 220.93 | 12.38 | 226.73 | 0.2837 | 1033.4 | 916.2 | |
| 0.71 | 3.81 | 0.37 | 1.97 | -17.50 | 220.98 | 12.42 | 223.92 | 0.2970 | 866.2 | 569.9 | |
| 5.58 | 438.22 | 2.88 | 224.81 | -16.93 | 220.58 | 12.03 | 224.47 | 0.2858 | 1136.4 | 40.8 | |
| 1.33 | -21.00 | 0.68 | -21.00 | -14.45 | 220.41 | 11.85 | 231.10 | 0.2567 | 1110.6 | 999999 | |
| 2.30 | -24.00 | 1.19 | -24.00 | -16.90 | 220.26 | 11.70 | 223.79 | 0.2817 | 1094.4 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -13.39 | 219.97 | 11.42 | 233.58 | 0.2404 | 813.0 | 680.5 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -15.93 | 219.75 | 11.20 | 225.17 | 0.2645 | 929.0 | 768.0 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -13.83 | 219.49 | 10.93 | 230.94 | 0.2382 | 243.0 | 256.4 | |
| 2.83 | -24.00 | 1.46 | -24.00 | -17.01 | 219.30 | 10.75 | 221.15 | 0.2722 | 1214.3 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.01 | -19.08 | 219.33 | 10.78 | 216.45 | 0.2987 | -734.0 | -682.6 | |
| 3.28 | -24.00 | 1.69 | -24.00 | -17.26 | 218.90 | 10.34 | 219.47 | 0.2710 | -556.5 | 999999 | |
| 0.00 | 2.48 | 0.00 | 1.29 | -19.18 | 218.95 | 10.39 | 215.29 | 0.2963 | -742.0 | -570.4 | |
| 1.77 | -24.00 | 0.91 | -24.00 | -15.58 | 218.72 | 10.16 | 223.46 | 0.2482 | -468.6 | 999999 | |
| 0.00 | 2.21 | 0.00 | 1.14 | -18.65 | 218.63 | 10.07 | 215.55 | 0.2862 | -777.0 | -696.2 | |
| 6.91 | -24.00 | 3.54 | -24.00 | -16.35 | 218.37 | 9.82 | 220.37 | 0.2537 | -946.9 | 999999 | |
| 6.73 | -24.00 | 3.44 | -24.00 | -15.92 | 218.35 | 9.80 | 221.48 | 0.2482 | -1098.9 | 999999 | |
| 0.00 | 2.57 | 0.00 | 1.31 | -15.46 | 217.98 | 9.43 | 221.69 | 0.2384 | -869.0 | -773.1 | |
| 0.00 | 2.83 | 0.00 | 1.45 | -15.83 | 218.00 | 9.44 | 220.70 | 0.2432 | -824.0 | -744.6 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -18.02 | 217.76 | 9.20 | 214.55 | 0.2693 | -998.0 | -794.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -17.80 | 217.71 | 9.16 | 214.91 | 0.2660 | -945.0 | -776.6 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -15.84 | 217.59 | 9.03 | 219.45 | 0.2387 | -868.0 | -686.0 | |
| 0.00 | 4.69 | 0.00 | 2.40 | -16.91 | 217.61 | 9.05 | 216.70 | 0.2529 | -1038.0 | -814.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -13.19 | 217.23 | 8.68 | 226.82 | 0.2023 | -995.0 | -820.7 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -15.41 | 217.25 | 8.70 | 219.61 | 0.2297 | -791.0 | -639.1 | |
| 0.00 | 3.19 | 0.00 | 1.62 | -15.93 | 217.15 | 8.59 | 217.82 | 0.2354 | -959.0 | -736.8 | |
| 0.00 | 1.68 | 0.00 | 0.89 | -23.69 | 216.54 | 7.99 | 201.94 | 0.3420 | -798.0 | -632.7 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -20.54 | 213.78 | 5.23 | 197.99 | 0.2775 | -996.0 | -765.3 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -18.41 | 211.65 | 3.09 | 192.74 | 0.2332 | -913.0 | -699.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -18.04 | 211.23 | 2.68 | 191.40 | 0.2256 | -750.0 | -646.4 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -18.44 | 211.17 | 2.62 | 190.81 | 0.2321 | -802.0 | -636.0 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -18.13 | 210.66 | 2.11 | 188.95 | 0.2255 | -784.0 | -799.7 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -21.49 | 210.67 | 2.11 | 187.03 | 0.2818 | -792.0 | -682.2 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -19.18 | 208.67 | 0.11 | 180.44 | 0.2406 | -889.0 | -651.1 | |
| 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. | |