SDO HMI 2011-12-05 15:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 97.99 | 427.56 | 54.82 | 239.61 | 7.41 | 131.31 | 26.58 | 286.16 | 0.4625 | 26.3 | 19.0 | |
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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 | 0.94 | 0.00 | 0.55 | 4.54 | 136.28 | 31.54 | 278.08 | 0.5288 | -649.0 | -474.4 | |
| 19.44 | 140.20 | 11.36 | 81.92 | 6.71 | 136.16 | 31.43 | 282.16 | 0.5319 | -1121.5 | -295.5 | |
| 1.11 | -2.00 | 0.64 | -2.00 | 6.89 | 135.76 | 31.02 | 282.64 | 0.5265 | -888.2 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.70 | 8.89 | 135.93 | 31.19 | 286.26 | 0.5351 | 721.0 | 572.1 | |
| 2.73 | -2.00 | 1.58 | -2.00 | 6.62 | 135.63 | 30.90 | 282.18 | 0.5239 | -932.6 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 5.73 | 135.06 | 30.32 | 280.67 | 0.5133 | -900.0 | -765.6 | |
| 0.00 | 1.19 | 0.00 | 0.69 | 5.94 | 135.07 | 30.33 | 281.06 | 0.5139 | -597.0 | -424.5 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 5.35 | 134.87 | 30.13 | 279.98 | 0.5095 | 359.0 | 365.7 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 6.95 | 134.93 | 30.20 | 283.05 | 0.5146 | -665.0 | -565.0 | |
| 0.00 | 1.79 | 0.00 | 1.03 | 5.70 | 134.85 | 30.11 | 280.67 | 0.5101 | -663.0 | -525.6 | |
| 24.05 | 45.11 | 13.84 | 25.95 | 6.56 | 134.80 | 30.07 | 282.36 | 0.5116 | -1034.3 | -543.6 | |
| 0.00 | 1.71 | 0.00 | 0.98 | 7.04 | 134.49 | 29.75 | 283.39 | 0.5084 | -863.0 | -598.0 | |
| 0.00 | 0.51 | 0.00 | 0.29 | 6.45 | 134.11 | 29.37 | 282.38 | 0.5010 | -892.0 | -817.8 | |
| 1.88 | 10.66 | 1.07 | 6.08 | 5.35 | 133.98 | 29.24 | 280.25 | 0.4963 | 707.2 | 168.6 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 5.85 | 134.00 | 29.27 | 281.24 | 0.4979 | -819.0 | -660.2 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 6.54 | 133.98 | 29.24 | 282.60 | 0.4993 | -690.0 | -643.9 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 5.20 | 133.56 | 28.82 | 280.08 | 0.4897 | -901.0 | -789.7 | |
| 0.00 | 2.47 | 0.00 | 1.38 | 5.95 | 131.62 | 26.88 | 282.32 | 0.4622 | -673.0 | -694.0 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 8.51 | 130.78 | 26.04 | 288.17 | 0.4590 | -734.0 | -599.8 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 7.47 | 129.98 | 25.25 | 286.40 | 0.4427 | -876.0 | -689.7 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 7.26 | 129.44 | 24.71 | 286.25 | 0.4337 | -863.0 | -705.5 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 7.62 | 129.37 | 24.63 | 287.10 | 0.4340 | 261.0 | 139.4 | |
| 0.00 | 2.98 | 0.00 | 1.64 | 8.28 | 128.98 | 24.25 | 288.81 | 0.4311 | 733.0 | 582.6 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 10.91 | 128.20 | 23.46 | 295.18 | 0.4338 | 755.0 | 560.8 | |
| 42.21 | 185.31 | 22.81 | 100.23 | 8.37 | 126.97 | 22.24 | 290.49 | 0.4014 | 1221.0 | 357.1 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 7.98 | 126.21 | 21.47 | 290.18 | 0.3879 | 711.0 | 610.9 | |
| 6.57 | 9.30 | 3.52 | 4.98 | 7.87 | 125.92 | 21.18 | 290.13 | 0.3828 | 1129.7 | 819.6 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 12.06 | 124.21 | 19.47 | 301.96 | 0.3858 | 662.0 | 453.3 | |
| 0.00 | 2.64 | 0.00 | 1.39 | 6.32 | 123.53 | 18.80 | 288.05 | 0.3383 | 823.0 | 648.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 8.85 | 123.40 | 18.66 | 295.11 | 0.3507 | 757.0 | 553.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 7.39 | 123.14 | 18.40 | 291.44 | 0.3378 | 853.0 | 635.9 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 7.01 | 122.62 | 17.88 | 290.87 | 0.3276 | 953.0 | 800.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 6.15 | 122.46 | 17.73 | 288.50 | 0.3206 | 832.0 | 607.9 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 6.50 | 122.41 | 17.68 | 289.60 | 0.3217 | 1033.0 | 870.3 | |
| 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. | |