SDO HMI 2011-10-25 20:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 222.51 | 1292.65 | 131.33 | 767.23 | 8.01 | 249.57 | -32.90 | 83.28 | 0.5411 | -161.1 | -59.2 | |
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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 | 0.66 | 8.82 | 258.47 | -24.01 | 79.62 | 0.4105 | -789.0 | -523.7 | |
| 0.00 | 1.56 | 0.00 | 0.85 | 11.24 | 258.21 | -24.26 | 73.97 | 0.4211 | -752.0 | -604.3 | |
| 0.00 | 1.13 | 0.00 | 0.62 | 11.65 | 258.04 | -24.44 | 73.10 | 0.4252 | -852.0 | -647.6 | |
| 0.00 | 1.30 | 0.00 | 0.73 | 11.34 | 255.43 | -27.04 | 75.00 | 0.4634 | -774.0 | -625.7 | |
| 100.89 | 668.45 | 55.92 | 371.51 | 6.48 | 255.72 | -26.75 | 85.57 | 0.4505 | -1448.8 | -445.5 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 9.24 | 255.35 | -27.12 | 79.54 | 0.4594 | 786.0 | 651.4 | |
| 0.00 | 1.74 | 0.00 | 0.97 | 8.97 | 255.38 | -27.10 | 80.12 | 0.4586 | 769.0 | 553.7 | |
| 3.21 | -5.00 | 1.79 | -5.00 | 6.94 | 255.35 | -27.12 | 84.58 | 0.4564 | -810.0 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 8.40 | 255.18 | -27.29 | 81.42 | 0.4606 | 629.0 | 398.6 | |
| 1.56 | -5.00 | 0.87 | -5.00 | 6.01 | 255.30 | -27.17 | 86.62 | 0.4568 | -947.8 | 999999 | |
| 2.78 | -5.00 | 1.55 | -5.00 | 5.77 | 255.32 | -27.15 | 87.14 | 0.4565 | -651.8 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.12 | 11.46 | 254.73 | -27.74 | 75.02 | 0.4742 | -877.0 | -647.7 | |
| 0.00 | 2.17 | 0.00 | 1.22 | 11.48 | 254.45 | -28.02 | 75.09 | 0.4783 | -809.0 | -697.6 | |
| 3.30 | -5.00 | 1.84 | -5.00 | 6.68 | 254.72 | -27.75 | 85.20 | 0.4660 | -701.0 | 999999 | |
| 1.13 | -5.00 | 0.63 | -5.00 | 6.43 | 254.43 | -28.04 | 85.76 | 0.4703 | -989.3 | 999999 | |
| 6.16 | -5.00 | 3.46 | -5.00 | 6.24 | 254.24 | -28.23 | 86.16 | 0.4732 | -1034.4 | 999999 | |
| 5.38 | -5.00 | 3.02 | -5.00 | 5.91 | 254.26 | -28.21 | 86.86 | 0.4729 | -848.1 | 999999 | |
| 2.60 | 3.39 | 1.46 | 1.90 | 3.85 | 254.22 | -28.25 | 91.22 | 0.4743 | 833.4 | 680.6 | |
| 0.61 | -5.00 | 0.34 | -5.00 | 5.78 | 254.03 | -28.44 | 87.13 | 0.4764 | -614.7 | 999999 | |
| 0.00 | 2.69 | 0.00 | 1.51 | 4.83 | 254.04 | -28.43 | 89.14 | 0.4764 | -754.0 | -666.6 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 8.28 | 253.83 | -28.64 | 81.91 | 0.4811 | 732.0 | 524.2 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 5.12 | 253.96 | -28.51 | 88.52 | 0.4775 | -479.0 | -494.8 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 7.68 | 253.77 | -28.70 | 83.17 | 0.4813 | -672.0 | -433.9 | |
| 0.00 | 1.30 | 0.00 | 0.75 | 12.56 | 252.86 | -29.61 | 73.56 | 0.5048 | -641.0 | -458.5 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 8.73 | 253.10 | -29.37 | 81.12 | 0.4927 | -645.0 | -492.1 | |
| 0.00 | 1.48 | 0.00 | 0.85 | 11.34 | 252.35 | -30.12 | 76.13 | 0.5089 | -811.0 | -595.7 | |
| 0.00 | 1.39 | 0.00 | 0.80 | 11.38 | 252.02 | -30.45 | 76.14 | 0.5137 | -819.0 | -672.0 | |
| 0.00 | 1.56 | 0.00 | 0.90 | 10.93 | 252.08 | -30.40 | 76.99 | 0.5119 | -749.0 | -517.7 | |
| 0.00 | 1.56 | 0.00 | 0.91 | 14.35 | 251.55 | -30.92 | 70.73 | 0.5295 | -810.0 | -581.6 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 5.57 | 251.76 | -30.71 | 87.56 | 0.5107 | -687.0 | -589.5 | |
| 0.00 | 1.65 | 0.00 | 0.95 | 6.05 | 251.25 | -31.23 | 86.61 | 0.5185 | -615.0 | -590.3 | |
| 0.00 | 0.61 | 0.00 | 0.35 | 5.42 | 251.28 | -31.19 | 87.83 | 0.5180 | -543.0 | -553.4 | |
| 1.48 | 2.87 | 0.86 | 1.66 | 6.36 | 250.91 | -31.56 | 86.02 | 0.5236 | -642.4 | -565.3 | |
| 0.35 | 1.39 | 0.20 | 0.82 | 7.51 | 249.83 | -32.64 | 83.91 | 0.5400 | -795.0 | -642.5 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 6.12 | 249.00 | -33.47 | 86.49 | 0.5515 | 673.0 | 468.2 | |
| 0.00 | 1.56 | 0.00 | 0.94 | 7.52 | 247.54 | -34.93 | 84.05 | 0.5729 | 730.0 | 586.3 | |
| 0.00 | 2.17 | 0.00 | 1.32 | 9.30 | 247.21 | -35.26 | 80.99 | 0.5790 | 889.0 | 780.4 | |
| 0.00 | 3.13 | 0.00 | 1.89 | 7.17 | 247.21 | -35.26 | 84.67 | 0.5775 | 903.0 | 691.1 | |
| 0.00 | 2.52 | 0.00 | 1.53 | 7.44 | 247.18 | -35.29 | 84.21 | 0.5780 | 795.0 | 701.6 | |
| 0.00 | 1.04 | 0.00 | 0.63 | 9.67 | 246.94 | -35.53 | 80.38 | 0.5832 | 755.0 | 692.5 | |
| 0.00 | 1.13 | 0.00 | 0.69 | 9.94 | 246.87 | -35.60 | 79.93 | 0.5846 | 692.0 | 611.5 | |
| 0.00 | 2.43 | 0.00 | 1.48 | 8.10 | 246.71 | -35.76 | 83.10 | 0.5850 | 796.0 | 673.4 | |
| 0.00 | 1.04 | 0.00 | 0.64 | 9.29 | 246.50 | -35.97 | 81.09 | 0.5889 | 688.0 | 567.1 | |
| 0.00 | 1.13 | 0.00 | 0.69 | 9.55 | 246.21 | -36.26 | 80.70 | 0.5933 | 715.0 | 594.4 | |
| 0.00 | 1.13 | 0.00 | 0.69 | 9.30 | 246.09 | -36.38 | 81.13 | 0.5947 | 578.0 | 439.8 | |
| 0.00 | 1.04 | 0.00 | 0.64 | 8.08 | 246.23 | -36.24 | 83.18 | 0.5918 | 569.0 | 466.8 | |
| 0.00 | 1.56 | 0.00 | 0.96 | 7.88 | 245.95 | -36.52 | 83.52 | 0.5956 | 620.0 | 486.4 | |
| 0.00 | 1.48 | 0.00 | 0.92 | 6.00 | 245.29 | -37.18 | 86.70 | 0.6042 | 522.0 | 445.6 | |
| 0.00 | 1.65 | 0.00 | 1.03 | 9.36 | 244.91 | -37.56 | 81.17 | 0.6110 | 732.0 | 616.2 | |
| 1.56 | 561.74 | 0.99 | 359.23 | 9.44 | 244.17 | -38.30 | 81.12 | 0.6211 | 828.5 | 316.7 | |
| 0.00 | 1.30 | 0.00 | 0.82 | 5.66 | 244.56 | -37.91 | 87.24 | 0.6144 | 517.0 | 425.6 | |
| 30.21 | -50.00 | 19.19 | -50.00 | 10.28 | 243.70 | -38.77 | 79.82 | 0.6283 | 1151.2 | 999999 | |
| 23.44 | -50.00 | 14.96 | -50.00 | 8.76 | 243.28 | -39.19 | 82.28 | 0.6325 | 1106.6 | 999999 | |
| 37.07 | -50.00 | 23.75 | -50.00 | 9.62 | 243.05 | -39.42 | 80.95 | 0.6362 | 1058.4 | 999999 | |
| 0.78 | -50.00 | 0.50 | -50.00 | 9.50 | 242.52 | -39.95 | 81.19 | 0.6432 | 510.3 | 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. | |