SDO HMI 2011-10-25 22:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 234.82 | 1278.98 | 137.69 | 749.54 | 8.00 | 249.60 | -31.77 | 83.20 | 0.5247 | -110.8 | -73.5 | |
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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 | 1.22 | 0.00 | 0.65 | 8.86 | 258.51 | -22.86 | 79.13 | 0.3925 | -793.0 | -549.5 | |
| 100.04 | 661.54 | 54.93 | 364.13 | 6.46 | 255.72 | -25.65 | 85.53 | 0.4333 | -1457.3 | -458.2 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 4.25 | 255.78 | -25.58 | 90.64 | 0.4325 | 519.0 | 393.9 | |
| 0.00 | 1.13 | 0.00 | 0.62 | 9.28 | 255.39 | -25.97 | 79.12 | 0.4420 | 778.0 | 626.8 | |
| 5.38 | -2.00 | 2.97 | -2.00 | 6.86 | 255.33 | -26.04 | 84.63 | 0.4396 | -916.3 | 999999 | |
| 0.43 | -2.00 | 0.24 | -2.00 | 5.99 | 255.31 | -26.06 | 86.61 | 0.4395 | -949.4 | 999999 | |
| 0.43 | -2.00 | 0.24 | -2.00 | 7.00 | 255.15 | -26.22 | 84.33 | 0.4425 | -839.0 | 999999 | |
| 0.00 | 2.52 | 0.00 | 1.41 | 11.43 | 254.42 | -26.95 | 74.76 | 0.4623 | -882.0 | -669.8 | |
| 0.00 | 1.04 | 0.00 | 0.58 | 7.72 | 254.30 | -27.07 | 82.85 | 0.4564 | -79.0 | -125.1 | |
| 10.25 | -2.00 | 5.70 | -2.00 | 6.25 | 254.25 | -27.11 | 86.08 | 0.4560 | -1034.5 | 999999 | |
| 2.26 | 3.21 | 1.25 | 1.79 | 3.90 | 254.36 | -27.01 | 91.27 | 0.4551 | 812.4 | 753.0 | |
| 5.91 | -2.00 | 3.28 | -2.00 | 5.86 | 254.24 | -27.13 | 86.93 | 0.4561 | -833.4 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.06 | 5.23 | 254.07 | -27.30 | 88.32 | 0.4588 | -573.0 | -411.8 | |
| 0.00 | 2.78 | 0.00 | 1.55 | 4.78 | 254.06 | -27.31 | 89.30 | 0.4592 | -887.0 | -660.1 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 8.44 | 253.84 | -27.53 | 81.35 | 0.4644 | 951.0 | 733.5 | |
| 0.00 | 1.56 | 0.00 | 0.87 | 7.75 | 253.65 | -27.72 | 82.88 | 0.4664 | -655.0 | -504.9 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 4.97 | 253.68 | -27.69 | 88.86 | 0.4650 | -547.0 | -311.9 | |
| 0.00 | 1.39 | 0.00 | 0.78 | 11.17 | 253.07 | -28.30 | 75.83 | 0.4816 | -816.0 | -692.8 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 12.33 | 252.87 | -28.50 | 73.54 | 0.4880 | -538.0 | -525.2 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 13.62 | 252.53 | -28.83 | 71.14 | 0.4973 | -795.0 | -643.6 | |
| 0.00 | 1.30 | 0.00 | 0.74 | 12.60 | 252.03 | -29.33 | 73.36 | 0.5010 | -647.0 | -493.6 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 11.40 | 252.00 | -29.36 | 75.75 | 0.4979 | -752.0 | -685.9 | |
| 0.00 | 1.04 | 0.00 | 0.60 | 14.33 | 251.52 | -29.85 | 70.26 | 0.5144 | -514.0 | -454.2 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 12.07 | 251.50 | -29.86 | 74.61 | 0.5071 | -564.0 | -408.3 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 4.46 | 252.06 | -29.30 | 89.83 | 0.4899 | -418.0 | -388.4 | |
| 0.00 | 1.39 | 0.00 | 0.79 | 5.50 | 251.88 | -29.49 | 87.71 | 0.4924 | -951.0 | -627.2 | |
| 0.00 | 1.48 | 0.00 | 0.84 | 5.42 | 251.40 | -29.97 | 87.86 | 0.4997 | -642.0 | -431.8 | |
| 0.00 | 3.73 | 0.00 | 2.13 | 6.04 | 251.33 | -30.04 | 86.61 | 0.5007 | -875.0 | -592.5 | |
| 0.00 | 1.82 | 0.00 | 1.04 | 6.51 | 251.23 | -30.14 | 85.66 | 0.5023 | -562.0 | -472.7 | |
| 2.00 | 3.82 | 1.15 | 2.19 | 6.38 | 250.96 | -30.41 | 85.94 | 0.5064 | -631.5 | -554.1 | |
| 0.00 | 1.22 | 0.00 | 0.71 | 7.53 | 249.82 | -31.55 | 83.78 | 0.5238 | -775.0 | -682.1 | |
| 0.00 | 1.56 | 0.00 | 0.93 | 10.17 | 247.44 | -33.93 | 79.24 | 0.5614 | 715.0 | 569.7 | |
| 0.00 | 2.17 | 0.00 | 1.29 | 7.54 | 247.67 | -33.69 | 83.91 | 0.5552 | 917.0 | 665.0 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 11.24 | 247.15 | -34.22 | 77.41 | 0.5673 | 728.0 | 648.5 | |
| 0.00 | 2.78 | 0.00 | 1.67 | 9.34 | 247.09 | -34.27 | 80.76 | 0.5652 | 810.0 | 751.2 | |
| 0.00 | 2.52 | 0.00 | 1.51 | 7.49 | 247.21 | -34.16 | 84.04 | 0.5619 | 879.0 | 706.3 | |
| 0.96 | 1.39 | 0.57 | 0.83 | 7.16 | 247.20 | -34.17 | 84.63 | 0.5619 | 834.0 | 798.4 | |
| 0.00 | 4.69 | 0.00 | 2.82 | 9.69 | 246.87 | -34.50 | 80.18 | 0.5688 | 523.0 | 692.3 | |
| 0.00 | 1.82 | 0.00 | 1.10 | 10.19 | 246.73 | -34.63 | 79.32 | 0.5714 | 687.0 | 485.0 | |
| 0.00 | 1.48 | 0.00 | 0.89 | 7.94 | 246.54 | -34.82 | 83.30 | 0.5717 | 647.0 | 512.0 | |
| 0.00 | 2.08 | 0.00 | 1.26 | 7.97 | 245.99 | -35.38 | 83.29 | 0.5796 | 769.0 | 581.1 | |
| 0.00 | 1.04 | 0.00 | 0.64 | 9.75 | 245.57 | -35.80 | 80.28 | 0.5871 | 500.0 | 400.6 | |
| 0.00 | 0.61 | 0.00 | 0.37 | 5.81 | 245.84 | -35.53 | 87.03 | 0.5811 | 595.0 | 486.7 | |
| 0.00 | 1.22 | 0.00 | 0.75 | 9.12 | 245.00 | -36.36 | 81.42 | 0.5943 | -347.0 | -313.4 | |
| 0.00 | 1.48 | 0.00 | 0.90 | 6.05 | 245.30 | -36.06 | 86.61 | 0.5886 | 555.0 | 504.0 | |
| 0.00 | 0.96 | 0.00 | 0.59 | 10.39 | 244.65 | -36.71 | 79.34 | 0.6006 | 724.0 | 603.3 | |
| 2.78 | 545.69 | 1.72 | 343.59 | 9.63 | 244.45 | -36.92 | 80.63 | 0.6024 | 828.5 | 323.4 | |
| 0.00 | 1.65 | 0.00 | 1.02 | 5.81 | 244.69 | -36.68 | 87.01 | 0.5973 | 672.0 | 475.6 | |
| 0.52 | -47.00 | 0.33 | -47.00 | 9.66 | 243.80 | -37.57 | 80.67 | 0.6114 | 875.8 | 999999 | |
| 36.30 | -47.00 | 22.72 | -47.00 | 10.34 | 243.67 | -37.70 | 79.57 | 0.6139 | 1142.3 | 999999 | |
| 21.71 | -47.00 | 13.64 | -47.00 | 8.76 | 243.30 | -38.07 | 82.19 | 0.6174 | 1136.7 | 999999 | |
| 43.77 | -47.00 | 27.63 | -47.00 | 9.58 | 243.00 | -38.36 | 80.88 | 0.6221 | 1038.2 | 999999 | |
| 1.04 | -47.00 | 0.66 | -47.00 | 8.42 | 243.11 | -38.26 | 82.75 | 0.6197 | 783.6 | 999999 | |
| 1.04 | -47.00 | 0.66 | -47.00 | 8.65 | 242.89 | -38.48 | 82.40 | 0.6229 | 517.0 | 999999 | |
| 0.00 | 1.74 | 0.00 | 1.11 | 10.31 | 241.96 | -39.40 | 79.86 | 0.6367 | 447.0 | 352.6 | |
| 0.00 | 1.22 | 0.00 | 0.81 | 10.35 | 239.43 | -41.93 | 80.09 | 0.6697 | 438.0 | 358.6 | |
| 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. | |