SDO HMI 2011-12-18 19:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.39 | 111.59 | 8.49 | 61.18 | 21.85 | 299.85 | 8.61 | 340.12 | 0.4308 | -97.1 | 21.1 | |
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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 | 1.53 | 0.00 | 0.85 | 19.36 | 309.30 | 18.07 | 320.28 | 0.4597 | -725.0 | -593.3 | |
| 0.00 | 1.79 | 0.00 | 0.99 | 19.58 | 308.80 | 17.56 | 321.36 | 0.4573 | -955.0 | -691.5 | |
| 0.00 | 2.30 | 0.00 | 1.27 | 18.63 | 308.37 | 17.13 | 320.63 | 0.4420 | -755.0 | -648.1 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 18.25 | 308.00 | 16.77 | 320.64 | 0.4339 | -815.0 | -613.3 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 18.44 | 307.83 | 16.59 | 321.22 | 0.4344 | -872.0 | -720.9 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 14.50 | 307.26 | 16.03 | 315.48 | 0.3829 | -761.0 | -583.3 | |
| 11.31 | 14.20 | 6.24 | 7.83 | 19.88 | 306.90 | 15.67 | 324.86 | 0.4431 | -899.6 | -685.6 | |
| 4.08 | 5.27 | 2.25 | 2.90 | 19.78 | 306.40 | 15.17 | 325.58 | 0.4374 | -950.1 | -733.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 19.90 | 304.99 | 13.76 | 328.25 | 0.4268 | 772.0 | 629.5 | |
| 0.00 | 2.38 | 0.00 | 1.29 | 18.92 | 304.30 | 13.06 | 328.24 | 0.4080 | -847.0 | -663.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 21.39 | 303.66 | 12.43 | 332.53 | 0.4364 | -782.0 | -569.2 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 20.49 | 303.23 | 12.00 | 332.31 | 0.4209 | -793.0 | -674.5 | |
| 0.00 | 1.87 | 0.00 | 1.02 | 20.24 | 303.18 | 11.95 | 332.11 | 0.4170 | -826.0 | -624.3 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 18.03 | 302.96 | 11.72 | 329.72 | 0.3849 | -723.0 | -655.1 | |
| 0.00 | 1.79 | 0.00 | 0.96 | 18.25 | 302.88 | 11.64 | 330.19 | 0.3873 | -791.0 | -622.5 | |
| 0.00 | 5.70 | 0.00 | 3.07 | 19.13 | 302.59 | 11.35 | 331.94 | 0.3972 | -805.0 | -712.6 | |
| 0.00 | 3.40 | 0.00 | 1.83 | 19.29 | 302.31 | 11.08 | 332.71 | 0.3973 | -876.0 | -797.4 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 18.12 | 301.70 | 10.46 | 332.56 | 0.3763 | -781.0 | -625.2 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 19.09 | 301.57 | 10.34 | 334.06 | 0.3892 | -314.0 | -398.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 19.31 | 301.42 | 10.19 | 334.63 | 0.3913 | -960.0 | -828.1 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 19.53 | 301.31 | 10.08 | 335.12 | 0.3937 | -653.0 | -543.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 27.47 | 301.00 | 9.77 | 342.63 | 0.5064 | -273.0 | -299.0 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 27.34 | 300.86 | 9.62 | 342.79 | 0.5038 | -764.0 | -611.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.50 | 300.26 | 9.03 | 337.39 | 0.3864 | -824.0 | -585.2 | |
| 0.00 | 2.47 | 0.00 | 1.33 | 20.64 | 300.07 | 8.84 | 338.95 | 0.4021 | -910.0 | -702.7 | |
| 0.00 | 1.70 | 0.00 | 0.90 | 18.27 | 299.32 | 8.08 | 338.27 | 0.3623 | -1048.0 | -884.7 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 18.74 | 298.65 | 7.41 | 340.38 | 0.3655 | -846.0 | -682.2 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 25.29 | 298.31 | 7.08 | 346.03 | 0.4634 | -664.0 | -521.2 | |
| 0.00 | 2.98 | 0.00 | 1.61 | 21.72 | 297.67 | 6.44 | 345.09 | 0.4066 | 760.0 | 637.1 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 22.29 | 297.22 | 5.98 | 346.45 | 0.4137 | 651.0 | 671.8 | |
| 0.00 | 2.38 | 0.00 | 1.30 | 22.49 | 296.97 | 5.74 | 347.11 | 0.4158 | 677.0 | 590.5 | |
| 0.00 | 4.25 | 0.00 | 2.31 | 22.19 | 296.38 | 5.15 | 348.23 | 0.4092 | 909.0 | 832.7 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 26.35 | 296.49 | 5.26 | 349.98 | 0.4735 | 770.0 | 580.4 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 26.85 | 296.38 | 5.15 | 350.38 | 0.4808 | 577.0 | 484.8 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 24.53 | 295.95 | 4.72 | 350.26 | 0.4442 | 605.0 | 482.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 24.20 | 295.84 | 4.61 | 350.34 | 0.4389 | 803.0 | 679.2 | |
| 0.00 | 2.64 | 0.00 | 1.43 | 21.97 | 295.48 | 4.25 | 350.14 | 0.4030 | 846.0 | 723.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 22.26 | 295.46 | 4.22 | 350.33 | 0.4075 | 634.0 | 531.8 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 24.14 | 295.23 | 3.99 | 351.59 | 0.4363 | 702.0 | 591.1 | |
| 0.00 | 3.74 | 0.00 | 2.02 | 21.68 | 294.96 | 3.73 | 351.20 | 0.3970 | 880.0 | 626.9 | |
| 0.00 | 3.15 | 0.00 | 1.69 | 21.52 | 294.64 | 3.41 | 351.89 | 0.3937 | 1025.0 | 934.1 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 23.00 | 294.65 | 3.41 | 352.42 | 0.4172 | 640.0 | 495.9 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.16 | 294.16 | 2.92 | 352.91 | 0.3871 | 866.0 | 693.5 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 28.88 | 294.25 | 3.01 | 354.77 | 0.5071 | 743.0 | 584.5 | |
| 0.00 | 2.30 | 0.00 | 1.33 | 30.08 | 294.22 | 2.98 | 355.06 | 0.5251 | 657.0 | 610.7 | |
| 0.00 | 2.13 | 0.00 | 1.24 | 30.46 | 294.13 | 2.89 | 355.28 | 0.5306 | 731.0 | 623.3 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 29.46 | 293.35 | 2.12 | 356.40 | 0.5148 | 765.0 | 591.9 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 24.23 | 292.93 | 1.70 | 356.42 | 0.4340 | 699.0 | 620.2 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 24.95 | 292.68 | 1.45 | 357.04 | 0.4452 | 830.0 | 634.6 | |
| 0.00 | 4.68 | 0.00 | 2.59 | 25.15 | 292.39 | 1.16 | 357.65 | 0.4480 | 708.0 | 644.9 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 31.30 | 291.42 | 0.19 | 359.70 | 0.5412 | 705.0 | 575.3 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 22.51 | 290.93 | -0.30 | 0.69 | 0.4058 | 729.0 | 436.0 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 21.74 | 288.90 | -2.33 | 5.52 | 0.3952 | 740.0 | 520.7 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 30.33 | 286.56 | -4.67 | 7.63 | 0.5314 | 359.0 | 339.9 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 30.15 | 286.50 | -4.73 | 7.78 | 0.5290 | 829.0 | 588.4 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 20.63 | 286.01 | -5.22 | 12.84 | 0.3849 | 435.0 | 387.0 | |
| 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. | |