SDO HMI 2011-10-26 12:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.27 | 162.26 | 10.80 | 82.72 | 16.08 | 279.49 | 5.80 | 335.23 | 0.2331 | -189.3 | -107.7 | |
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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 | 2.34 | 0.00 | 1.23 | 12.99 | 290.76 | 17.07 | 296.69 | 0.3215 | -824.0 | -655.6 | |
| 0.00 | 1.30 | 0.00 | 0.68 | 12.54 | 290.70 | 17.00 | 295.47 | 0.3176 | -768.0 | -653.7 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 13.91 | 290.51 | 16.81 | 299.58 | 0.3243 | -790.0 | -637.2 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 12.88 | 290.34 | 16.64 | 296.91 | 0.3145 | -829.0 | -697.7 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 17.05 | 289.70 | 16.01 | 308.93 | 0.3404 | -689.0 | -531.3 | |
| 0.00 | 1.30 | 0.00 | 0.68 | 16.87 | 289.49 | 15.80 | 308.85 | 0.3360 | -682.0 | -589.7 | |
| 0.00 | 9.64 | 0.00 | 5.00 | 14.07 | 288.76 | 15.07 | 302.63 | 0.3008 | -878.0 | -661.9 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 13.56 | 288.57 | 14.88 | 301.45 | 0.2939 | -784.0 | -695.6 | |
| 0.00 | 1.48 | 0.00 | 0.77 | 14.50 | 288.22 | 14.53 | 304.80 | 0.2970 | -831.0 | -664.1 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 13.85 | 287.70 | 14.01 | 303.80 | 0.2841 | -766.0 | -696.4 | |
| 0.00 | 1.48 | 0.00 | 0.76 | 13.19 | 287.28 | 13.59 | 302.52 | 0.2726 | -860.0 | -664.7 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 12.80 | 287.20 | 13.51 | 301.42 | 0.2681 | -843.0 | -642.4 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 14.61 | 285.95 | 12.25 | 309.58 | 0.2677 | -819.0 | -614.6 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 14.37 | 285.40 | 11.71 | 310.12 | 0.2582 | -854.0 | -722.5 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 13.16 | 283.75 | 10.06 | 310.32 | 0.2240 | -881.0 | -659.1 | |
| 0.00 | 3.04 | 0.00 | 1.56 | 17.96 | 280.82 | 7.13 | 332.41 | 0.2561 | -880.0 | -744.0 | |
| 20.75 | 42.63 | 10.54 | 21.66 | 16.05 | 280.25 | 6.56 | 330.40 | 0.2232 | -1164.6 | -585.2 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 18.03 | 279.94 | 6.25 | 335.49 | 0.2506 | -859.0 | -724.5 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 18.40 | 279.77 | 6.07 | 336.72 | 0.2550 | -753.0 | -651.8 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 21.02 | 279.83 | 6.14 | 340.20 | 0.2962 | -825.0 | -654.6 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 19.14 | 279.73 | 6.03 | 337.99 | 0.2662 | -780.0 | -711.2 | |
| 0.00 | 2.26 | 0.00 | 1.16 | 18.31 | 279.54 | 5.85 | 337.34 | 0.2522 | -1027.0 | -874.7 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 18.10 | 279.50 | 5.81 | 337.12 | 0.2486 | -1068.0 | -949.6 | |
| 0.52 | 7.90 | 0.26 | 3.99 | 15.00 | 278.82 | 5.13 | 333.74 | 0.1960 | -1131.8 | -873.8 | |
| 0.00 | 2.17 | 0.00 | 1.10 | 15.54 | 278.83 | 5.14 | 334.91 | 0.2045 | -681.0 | -589.7 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 14.79 | 278.72 | 5.03 | 333.68 | 0.1920 | -870.0 | -777.0 | |
| 0.00 | 4.08 | 0.00 | 2.05 | 14.13 | 278.28 | 4.58 | 334.15 | 0.1785 | -755.0 | -657.9 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 18.14 | 277.96 | 4.27 | 342.80 | 0.2403 | -492.0 | -385.1 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 13.95 | 277.78 | 4.09 | 336.19 | 0.1721 | -1006.0 | -760.0 | |
| 0.00 | 6.86 | 0.00 | 3.48 | 16.95 | 277.72 | 4.02 | 342.14 | 0.2198 | 675.0 | 289.6 | |
| 0.00 | 2.86 | 0.00 | 1.45 | 16.68 | 276.93 | 3.24 | 345.12 | 0.2116 | 753.0 | 654.2 | |
| 0.00 | 5.73 | 0.00 | 2.92 | 17.78 | 276.86 | 3.16 | 346.70 | 0.2294 | 1062.0 | 816.4 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 16.47 | 276.68 | 2.98 | 345.98 | 0.2070 | 732.0 | 607.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | 13.11 | 276.60 | 2.91 | 340.84 | 0.1513 | 881.0 | 655.9 | |
| 0.00 | 1.39 | 0.00 | 0.69 | 9.36 | 276.50 | 2.81 | 327.94 | 0.0916 | 980.0 | 734.8 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 17.63 | 276.48 | 2.78 | 348.10 | 0.2255 | 1044.0 | 907.4 | |
| 0.00 | 3.56 | 0.00 | 1.80 | 16.68 | 276.40 | 2.71 | 347.47 | 0.2095 | 912.0 | 851.9 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 17.81 | 276.29 | 2.60 | 349.03 | 0.2280 | 985.0 | 805.1 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 17.38 | 276.26 | 2.56 | 348.81 | 0.2207 | 1113.0 | 932.5 | |
| 0.00 | 5.12 | 0.00 | 2.59 | 16.26 | 276.21 | 2.52 | 347.89 | 0.2017 | 749.0 | 638.8 | |
| 0.00 | 2.34 | 0.00 | 1.19 | 17.26 | 276.00 | 2.31 | 349.78 | 0.2179 | 966.0 | 831.9 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 17.44 | 275.94 | 2.25 | 350.19 | 0.2208 | 808.0 | 622.0 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 18.39 | 275.80 | 2.11 | 351.48 | 0.2364 | 740.0 | 550.7 | |
| 0.00 | 2.86 | 0.00 | 1.46 | 18.70 | 275.39 | 1.70 | 353.26 | 0.2406 | 642.0 | 574.2 | |
| 0.00 | 1.22 | 0.00 | 0.61 | 12.00 | 274.70 | 1.01 | 352.05 | 0.1248 | 802.0 | 522.9 | |
| 0.00 | 1.22 | 0.00 | 0.61 | 15.65 | 274.56 | 0.87 | 355.51 | 0.1873 | 894.0 | 653.9 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 21.32 | 274.24 | 0.55 | 358.20 | 0.2835 | 938.0 | 790.3 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 11.67 | 271.96 | -1.73 | 14.17 | 0.1215 | 845.0 | 647.9 | |
| 0.00 | 1.74 | 0.00 | 0.87 | 13.38 | 271.61 | -2.08 | 13.52 | 0.1518 | 856.0 | 614.9 | |
| 0.00 | 3.99 | 0.00 | 2.04 | 19.19 | 271.20 | -2.49 | 9.46 | 0.2507 | 1019.0 | 728.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 14.19 | 270.31 | -3.38 | 19.55 | 0.1716 | 788.0 | 686.0 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 16.49 | 270.03 | -3.67 | 17.01 | 0.2106 | 704.0 | 580.4 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.64 | 269.25 | -4.45 | 20.10 | 0.2172 | 832.0 | 574.9 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 16.91 | 268.86 | -4.83 | 21.20 | 0.2238 | 850.0 | 554.8 | |
| 0.00 | 1.48 | 0.00 | 0.77 | 23.23 | 267.59 | -6.10 | 17.27 | 0.3306 | 925.0 | 762.3 | |
| 0.00 | 1.74 | 0.00 | 0.91 | 23.01 | 267.60 | -6.09 | 17.46 | 0.3272 | 844.0 | 682.5 | |
| 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. | |