SDO HMI 2011-06-04 23:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.35 | 348.66 | 32.52 | 204.24 | -22.09 | 35.01 | 24.23 | 225.52 | 0.5359 | -11.5 | -94.0 | |
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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 | 1.45 | 0.00 | 0.90 | -21.88 | 41.77 | 31.00 | 232.31 | 0.6061 | 769.0 | 593.4 | |
| 19.35 | 65.20 | 11.49 | 38.75 | -19.32 | 38.83 | 28.05 | 233.60 | 0.5535 | 1009.0 | 310.9 | |
| 0.00 | 2.53 | 0.00 | 1.49 | -18.42 | 38.52 | 27.74 | 234.73 | 0.5431 | 471.0 | 284.9 | |
| 0.00 | 2.98 | 0.00 | 1.75 | -18.71 | 38.03 | 27.25 | 233.83 | 0.5394 | 569.0 | 490.8 | |
| 0.00 | 5.52 | 0.00 | 3.36 | -23.60 | 38.35 | 27.58 | 226.91 | 0.5831 | 666.0 | 638.8 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -19.38 | 37.10 | 26.32 | 231.88 | 0.5338 | 754.0 | 583.8 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -23.40 | 37.78 | 27.01 | 226.64 | 0.5754 | 708.0 | 543.0 | |
| 0.00 | 3.17 | 0.00 | 1.85 | -19.61 | 36.92 | 26.15 | 231.35 | 0.5336 | 949.0 | 716.9 | |
| 0.00 | 3.35 | 0.00 | 1.97 | -20.68 | 36.97 | 26.20 | 229.76 | 0.5432 | 697.0 | 624.2 | |
| 0.00 | 2.62 | 0.00 | 1.53 | -19.84 | 36.78 | 26.01 | 230.86 | 0.5339 | 942.0 | 754.7 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -20.39 | 36.88 | 26.11 | 230.11 | 0.5397 | 764.0 | 686.2 | |
| 0.00 | 3.35 | 0.00 | 1.95 | -20.78 | 35.58 | 24.81 | 228.17 | 0.5285 | 864.0 | 547.3 | |
| 0.00 | 1.45 | 0.00 | 0.88 | -25.44 | 36.12 | 25.34 | 222.22 | 0.5774 | 859.0 | 703.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -19.55 | 34.91 | 24.14 | 229.35 | 0.5100 | -652.0 | -506.7 | |
| 0.45 | 1.72 | 0.27 | 1.02 | -23.70 | 35.52 | 24.75 | 223.89 | 0.5550 | 803.2 | 662.2 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -24.13 | 35.32 | 24.54 | 223.08 | 0.5570 | -204.0 | -184.3 | |
| 0.00 | 6.42 | 0.00 | 3.84 | -24.73 | 35.29 | 24.52 | 222.26 | 0.5627 | -732.0 | -573.7 | |
| 0.00 | 3.17 | 0.00 | 1.90 | -25.27 | 35.37 | 24.60 | 221.64 | 0.5686 | -565.0 | -473.8 | |
| 0.00 | 14.83 | 0.00 | 8.78 | -23.70 | 35.01 | 24.23 | 223.33 | 0.5498 | -5.0 | 99.6 | |
| 5.52 | 116.84 | 3.22 | 67.90 | -22.31 | 34.38 | 23.61 | 224.58 | 0.5300 | 801.7 | -150.4 | |
| 1.36 | -20.00 | 0.79 | -20.00 | -22.68 | 34.45 | 23.68 | 224.13 | 0.5342 | 573.2 | 999999 | |
| 1.18 | 7.69 | 0.69 | 4.53 | -23.70 | 34.50 | 23.73 | 222.76 | 0.5447 | -684.6 | -436.4 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -20.45 | 33.93 | 23.15 | 226.81 | 0.5072 | -740.0 | -561.7 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -21.63 | 34.05 | 23.27 | 225.19 | 0.5198 | 761.0 | 601.4 | |
| 0.00 | 2.17 | 0.00 | 1.29 | -24.27 | 34.54 | 23.76 | 222.04 | 0.5507 | -508.0 | -397.5 | |
| 6.42 | -20.00 | 3.75 | -20.00 | -22.58 | 34.15 | 23.37 | 223.92 | 0.5301 | 871.5 | 999999 | |
| 1.72 | 2.17 | 1.00 | 1.26 | -22.02 | 33.90 | 23.13 | 224.44 | 0.5221 | 727.5 | 665.8 | |
| 11.21 | 27.31 | 6.62 | 16.09 | -24.07 | 34.13 | 23.36 | 221.85 | 0.5447 | -875.9 | -254.8 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -22.18 | 33.68 | 22.91 | 223.95 | 0.5214 | 622.0 | 525.1 | |
| 0.00 | 2.71 | 0.00 | 1.56 | -21.14 | 33.19 | 22.41 | 224.90 | 0.5059 | -790.0 | -669.8 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -24.33 | 33.46 | 22.69 | 220.71 | 0.5409 | -773.0 | -657.1 | |
| 0.00 | 4.43 | 0.00 | 2.59 | -23.64 | 33.19 | 22.41 | 221.32 | 0.5311 | -191.0 | -111.0 | |
| 3.35 | 11.21 | 1.92 | 6.44 | -21.69 | 32.78 | 22.01 | 223.58 | 0.5071 | -831.1 | -718.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -24.54 | 33.10 | 22.33 | 220.01 | 0.5396 | -678.0 | -511.8 | |
| 0.00 | 2.35 | 0.00 | 1.37 | -23.77 | 32.96 | 22.19 | 220.87 | 0.5302 | -497.0 | -371.8 | |
| 0.00 | 6.24 | 0.00 | 3.63 | -23.47 | 32.87 | 22.10 | 221.16 | 0.5263 | -306.0 | -373.3 | |
| 4.79 | -20.00 | 2.77 | -20.00 | -22.68 | 32.70 | 21.92 | 222.05 | 0.5163 | -1038.5 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.28 | 32.53 | 21.75 | 222.40 | 0.5105 | -967.0 | -767.7 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -21.50 | 32.29 | 21.52 | 223.25 | 0.5001 | -804.0 | -631.2 | |
| 0.00 | 3.26 | 0.00 | 1.89 | -23.31 | 32.56 | 21.78 | 221.00 | 0.5214 | -737.0 | -681.5 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -23.54 | 32.52 | 21.75 | 220.65 | 0.5236 | -681.0 | -579.3 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -24.10 | 32.59 | 21.81 | 219.97 | 0.5301 | -563.0 | -492.9 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.02 | 32.24 | 21.46 | 222.41 | 0.5049 | -821.0 | -733.7 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -21.40 | 32.07 | 21.29 | 223.11 | 0.4967 | -896.0 | -761.0 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -22.25 | 32.20 | 21.43 | 222.04 | 0.5069 | -1029.0 | -885.3 | |
| 0.00 | 2.17 | 0.00 | 1.25 | -22.38 | 32.15 | 21.38 | 221.79 | 0.5078 | -788.0 | -711.9 | |
| 0.00 | 10.13 | 0.00 | 5.85 | -23.04 | 32.23 | 21.45 | 220.96 | 0.5154 | -600.0 | -613.8 | |
| 0.00 | 2.26 | 0.00 | 1.30 | -22.55 | 32.04 | 21.26 | 221.41 | 0.5084 | -697.0 | -577.7 | |
| 0.00 | 2.17 | 0.00 | 1.24 | -21.43 | 31.79 | 21.02 | 222.71 | 0.4942 | -721.0 | -695.3 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -22.81 | 31.97 | 21.20 | 220.96 | 0.5105 | -639.0 | -532.4 | |
| 0.00 | 1.81 | 0.00 | 1.04 | -22.35 | 31.79 | 21.02 | 221.38 | 0.5038 | -740.0 | -642.2 | |
| 0.00 | 1.81 | 0.00 | 1.04 | -22.61 | 31.77 | 20.99 | 220.97 | 0.5064 | -812.0 | -568.7 | |
| 0.00 | 1.81 | 0.00 | 1.03 | -21.86 | 31.30 | 20.52 | 221.44 | 0.4936 | -815.0 | -639.5 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -24.54 | 31.55 | 20.78 | 218.10 | 0.5251 | -576.0 | -419.1 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -25.11 | 29.72 | 18.95 | 214.96 | 0.5153 | -669.0 | -566.6 | |
| 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. | |