SDO HMI 2011-06-04 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.42 | 338.97 | 31.17 | 197.02 | -22.15 | 34.94 | 23.06 | 224.09 | 0.5239 | 58.3 | -72.0 | |
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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 | 0.90 | 0.00 | 0.56 | -22.09 | 42.20 | 30.32 | 231.47 | 0.6001 | 478.0 | 401.5 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -21.83 | 41.95 | 30.07 | 231.63 | 0.5954 | 583.0 | 459.1 | |
| 0.00 | 2.62 | 0.00 | 1.61 | -21.89 | 41.66 | 29.78 | 231.30 | 0.5927 | 777.0 | 652.3 | |
| 18.35 | 55.97 | 10.79 | 32.92 | -19.33 | 38.84 | 26.96 | 232.59 | 0.5407 | 1045.5 | 385.2 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -18.59 | 38.18 | 26.29 | 233.12 | 0.5270 | 570.0 | 458.8 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -24.18 | 39.14 | 27.26 | 225.83 | 0.5847 | 531.0 | 428.7 | |
| 0.90 | 6.78 | 0.55 | 4.09 | -23.71 | 38.40 | 26.52 | 225.74 | 0.5730 | 736.4 | 637.0 | |
| 0.00 | 1.90 | 0.00 | 1.14 | -23.02 | 38.18 | 26.29 | 226.47 | 0.5644 | 662.0 | 461.6 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -19.30 | 37.04 | 25.16 | 230.85 | 0.5195 | 759.0 | 606.6 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -19.62 | 36.95 | 25.07 | 230.25 | 0.5212 | 880.0 | 829.3 | |
| 0.00 | 2.35 | 0.00 | 1.37 | -20.66 | 37.06 | 25.18 | 228.76 | 0.5315 | 676.0 | 601.6 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -20.47 | 37.03 | 25.15 | 229.02 | 0.5294 | 618.0 | 551.0 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -20.30 | 36.93 | 25.05 | 229.16 | 0.5268 | 823.0 | 741.9 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -19.88 | 36.78 | 24.90 | 229.66 | 0.5215 | 901.0 | 784.1 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -20.30 | 36.32 | 24.44 | 228.51 | 0.5200 | 434.0 | 477.9 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -22.16 | 36.47 | 24.59 | 225.90 | 0.5387 | 772.0 | 581.9 | |
| 0.99 | 2.98 | 0.57 | 1.72 | -20.79 | 35.58 | 23.70 | 226.95 | 0.5163 | 670.3 | 654.3 | |
| 0.00 | 1.54 | 0.00 | 0.92 | -25.45 | 36.18 | 24.30 | 221.10 | 0.5675 | 809.0 | 740.6 | |
| 0.00 | 4.61 | 0.00 | 2.67 | -21.22 | 35.30 | 23.42 | 225.98 | 0.5172 | 573.0 | 567.9 | |
| 1.72 | 2.53 | 1.01 | 1.49 | -23.78 | 35.51 | 23.63 | 222.56 | 0.5444 | 760.4 | 597.2 | |
| 0.00 | 7.69 | 0.00 | 4.56 | -24.71 | 35.37 | 23.49 | 221.15 | 0.5523 | -658.0 | -548.6 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -23.52 | 35.10 | 23.22 | 222.45 | 0.5377 | 389.0 | 204.6 | |
| 0.00 | 3.35 | 0.00 | 1.99 | -25.25 | 35.37 | 23.49 | 220.45 | 0.5577 | -611.0 | -497.3 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -21.31 | 34.53 | 22.65 | 224.94 | 0.5100 | 660.0 | 487.7 | |
| 1.36 | 130.83 | 0.79 | 75.48 | -22.66 | 34.51 | 22.63 | 222.96 | 0.5231 | 547.9 | -101.8 | |
| 3.71 | -25.00 | 2.14 | -25.00 | -22.26 | 34.37 | 22.49 | 223.35 | 0.5177 | 878.7 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.12 | -24.25 | 34.66 | 22.78 | 220.94 | 0.5407 | -454.0 | -371.7 | |
| 1.08 | 1.90 | 0.62 | 1.09 | -21.61 | 34.12 | 22.24 | 224.00 | 0.5086 | 621.8 | 538.1 | |
| 0.90 | 13.65 | 0.53 | 8.00 | -23.68 | 34.48 | 22.60 | 221.50 | 0.5332 | -679.1 | -203.3 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -20.47 | 33.91 | 22.03 | 225.46 | 0.4949 | -780.0 | -601.1 | |
| 5.15 | -25.00 | 2.98 | -25.00 | -22.53 | 34.20 | 22.32 | 222.77 | 0.5187 | 907.0 | 999999 | |
| 0.00 | 2.89 | 0.00 | 1.67 | -22.00 | 33.97 | 22.09 | 223.25 | 0.5110 | 888.0 | 714.4 | |
| 12.30 | 29.57 | 7.20 | 17.28 | -24.08 | 34.19 | 22.31 | 220.61 | 0.5345 | -906.9 | -314.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -22.17 | 33.72 | 21.84 | 222.69 | 0.5100 | 541.0 | 468.6 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -23.58 | 33.64 | 21.76 | 220.61 | 0.5240 | -139.0 | -111.3 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -21.22 | 33.15 | 21.26 | 223.36 | 0.4944 | -984.0 | -792.3 | |
| 0.00 | 1.81 | 0.00 | 1.05 | -23.55 | 33.49 | 21.61 | 220.47 | 0.5222 | -252.0 | -223.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -24.28 | 33.44 | 21.56 | 219.42 | 0.5294 | -760.0 | -633.4 | |
| 0.00 | 2.08 | 0.00 | 1.18 | -21.32 | 32.95 | 21.07 | 222.96 | 0.4933 | -819.0 | -619.6 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -23.92 | 33.34 | 21.46 | 219.79 | 0.5246 | -671.0 | -529.0 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -21.94 | 32.94 | 21.06 | 222.04 | 0.4997 | -215.0 | -217.0 | |
| 1.54 | -25.00 | 0.88 | -25.00 | -22.36 | 32.83 | 20.95 | 221.29 | 0.5031 | -952.4 | 999999 | |
| 0.00 | 11.75 | 0.00 | 6.70 | -21.74 | 32.70 | 20.82 | 222.01 | 0.4952 | -942.0 | -807.3 | |
| 5.42 | -25.00 | 3.11 | -25.00 | -22.66 | 32.67 | 20.78 | 220.65 | 0.5047 | -1024.7 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -22.20 | 32.45 | 20.57 | 221.03 | 0.4976 | -910.0 | -802.8 | |
| 0.00 | 6.51 | 0.00 | 3.75 | -23.25 | 32.59 | 20.70 | 219.72 | 0.5103 | -826.0 | -701.4 | |
| 0.00 | 4.07 | 0.00 | 2.31 | -22.10 | 32.16 | 20.28 | 220.78 | 0.4936 | -889.0 | -772.9 | |
| 0.00 | 2.80 | 0.00 | 1.61 | -23.15 | 32.29 | 20.41 | 219.47 | 0.5063 | -694.0 | -599.5 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -22.92 | 32.25 | 20.37 | 219.74 | 0.5034 | -795.0 | -679.5 | |
| 0.00 | 2.35 | 0.00 | 1.34 | -22.36 | 32.09 | 20.21 | 220.31 | 0.4958 | -759.0 | -612.9 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -22.00 | 31.83 | 19.95 | 220.47 | 0.4893 | -867.0 | -748.0 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -21.74 | 31.72 | 19.84 | 220.70 | 0.4853 | -986.0 | -787.7 | |
| 0.00 | 2.53 | 0.00 | 1.44 | -22.27 | 31.76 | 19.88 | 220.01 | 0.4915 | -704.0 | -618.0 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -22.59 | 31.74 | 19.86 | 219.52 | 0.4949 | -787.0 | -586.5 | |
| 0.00 | 2.71 | 0.00 | 1.53 | -21.87 | 31.36 | 19.48 | 220.01 | 0.4832 | -822.0 | -767.0 | |
| 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. | |