SDO HMI 2011-10-26 08:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.02 | 178.59 | 12.66 | 90.61 | 16.11 | 278.77 | 2.89 | 347.13 | 0.2133 | -61.9 | -58.1 | |
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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 | 1.39 | 0.00 | 0.72 | 12.64 | 290.93 | 15.04 | 298.34 | 0.2890 | -769.0 | -425.8 | |
| 0.00 | 2.52 | 0.00 | 1.30 | 13.46 | 290.72 | 14.84 | 301.16 | 0.2924 | -763.0 | -737.5 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 12.58 | 290.64 | 14.76 | 298.60 | 0.2844 | -839.0 | -781.0 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 13.85 | 290.59 | 14.71 | 302.56 | 0.2938 | -738.0 | -575.4 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 13.92 | 290.37 | 14.49 | 303.12 | 0.2913 | -822.0 | -723.5 | |
| 0.00 | 3.04 | 0.00 | 1.56 | 14.16 | 288.56 | 12.67 | 307.31 | 0.2686 | -779.0 | -671.7 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 14.01 | 288.48 | 12.60 | 307.00 | 0.2662 | -1029.0 | -886.7 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 14.53 | 288.20 | 12.31 | 309.19 | 0.2676 | -771.0 | -629.6 | |
| 0.00 | 1.74 | 0.00 | 0.89 | 14.69 | 285.79 | 9.91 | 315.68 | 0.2392 | -747.0 | -645.1 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 14.34 | 285.31 | 9.42 | 315.98 | 0.2293 | -978.0 | -808.1 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 15.30 | 285.32 | 9.43 | 318.83 | 0.2412 | -827.0 | -708.5 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 21.26 | 284.68 | 8.80 | 333.17 | 0.3171 | 883.0 | 710.8 | |
| 0.00 | 1.30 | 0.00 | 0.68 | 21.45 | 284.59 | 8.71 | 333.67 | 0.3192 | 824.0 | 639.3 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 13.24 | 283.74 | 7.86 | 317.43 | 0.1977 | -957.0 | -748.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.34 | 282.76 | 6.87 | 324.67 | 0.2015 | -718.0 | -589.9 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 18.15 | 280.78 | 4.90 | 340.46 | 0.2437 | -773.0 | -619.3 | |
| 22.58 | 47.43 | 11.43 | 24.01 | 16.08 | 280.23 | 4.35 | 339.36 | 0.2075 | -1183.3 | -574.8 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 18.13 | 279.99 | 4.11 | 343.37 | 0.2391 | -776.0 | -587.7 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 18.96 | 279.76 | 3.88 | 345.20 | 0.2516 | -879.0 | -662.1 | |
| 0.00 | 7.56 | 0.00 | 3.85 | 18.07 | 279.24 | 3.36 | 346.23 | 0.2348 | -919.0 | -729.4 | |
| 1.22 | 22.32 | 0.61 | 11.25 | 15.24 | 278.91 | 3.03 | 344.08 | 0.1867 | -904.9 | -785.0 | |
| 0.00 | 1.65 | 0.00 | 0.83 | 14.37 | 278.78 | 2.89 | 343.37 | 0.1715 | -1025.0 | -776.0 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 16.70 | 278.28 | 2.40 | 348.88 | 0.2085 | -759.0 | -449.1 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 17.10 | 277.94 | 2.06 | 350.74 | 0.2142 | -483.0 | -382.2 | |
| 1.22 | 4.43 | 0.62 | 2.24 | 16.67 | 277.81 | 1.93 | 350.98 | 0.2066 | -579.6 | -297.9 | |
| 0.00 | 2.52 | 0.00 | 1.26 | 14.01 | 277.76 | 1.87 | 348.60 | 0.1613 | -926.0 | -741.1 | |
| 0.00 | 2.17 | 0.00 | 1.10 | 17.01 | 277.75 | 1.87 | 351.50 | 0.2121 | 678.0 | 543.4 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.56 | 277.72 | 1.83 | 346.74 | 0.1367 | 748.0 | 621.3 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 14.76 | 277.36 | 1.48 | 351.67 | 0.1730 | 1028.0 | 789.4 | |
| 0.00 | 0.43 | 0.00 | 0.22 | 16.67 | 277.25 | 1.37 | 353.57 | 0.2054 | 625.0 | 605.2 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 17.86 | 276.98 | 1.10 | 355.34 | 0.2252 | 750.0 | 561.2 | |
| 0.00 | 2.52 | 0.00 | 1.28 | 17.68 | 276.79 | 0.91 | 356.08 | 0.2218 | 1088.0 | 916.2 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 17.89 | 276.73 | 0.85 | 356.41 | 0.2254 | 876.0 | 753.7 | |
| 0.00 | 3.39 | 0.00 | 1.71 | 16.58 | 276.38 | 0.50 | 357.64 | 0.2027 | 1099.0 | 938.5 | |
| 0.00 | 16.68 | 0.00 | 8.47 | 17.56 | 276.35 | 0.47 | 357.95 | 0.2194 | 1133.0 | 787.7 | |
| 0.00 | 1.56 | 0.00 | 0.78 | 10.28 | 276.28 | 0.39 | 355.84 | 0.0936 | 927.0 | 675.8 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 17.25 | 275.91 | 0.03 | 359.86 | 0.2140 | 1071.0 | 894.8 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 17.47 | 275.88 | 0.00 | 0.00 | 0.2177 | 827.0 | 726.3 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 16.71 | 275.85 | -0.03 | 0.15 | 0.2046 | 865.0 | 681.1 | |
| 0.00 | 2.26 | 0.00 | 1.13 | 13.10 | 275.82 | -0.06 | 0.42 | 0.1424 | 797.0 | 570.0 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 18.63 | 275.47 | -0.41 | 1.64 | 0.2376 | 954.0 | 703.6 | |
| 0.00 | 1.48 | 0.00 | 0.76 | 21.22 | 274.92 | -0.96 | 3.19 | 0.2818 | 1009.0 | 776.1 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 11.66 | 274.64 | -1.25 | 10.34 | 0.1193 | 878.0 | 660.6 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 11.09 | 274.61 | -1.28 | 11.54 | 0.1096 | 819.0 | 605.5 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 15.34 | 274.52 | -1.36 | 7.23 | 0.1825 | 840.0 | 690.7 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 21.44 | 274.15 | -1.73 | 5.65 | 0.2864 | 773.0 | 572.3 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 23.16 | 274.10 | -1.78 | 5.23 | 0.3151 | 788.0 | 657.8 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 21.37 | 273.96 | -1.92 | 6.30 | 0.2857 | 920.0 | 761.4 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.59 | 273.99 | -1.89 | 13.63 | 0.1374 | 863.0 | 713.1 | |
| 0.00 | 1.48 | 0.00 | 0.74 | 10.67 | 272.97 | -2.91 | 26.61 | 0.1120 | 882.0 | 618.5 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 17.85 | 271.94 | -3.95 | 16.34 | 0.2339 | 982.0 | 750.8 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 11.56 | 271.87 | -4.02 | 30.78 | 0.1348 | 854.0 | 659.3 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 13.45 | 271.62 | -4.26 | 26.03 | 0.1655 | 823.0 | 537.0 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 19.26 | 271.11 | -4.77 | 17.61 | 0.2607 | 940.0 | 781.4 | |
| 0.00 | 4.69 | 0.00 | 2.37 | 13.94 | 268.53 | -7.36 | 38.39 | 0.2010 | 203.0 | 329.5 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 23.20 | 267.52 | -8.36 | 23.06 | 0.3427 | 900.0 | 771.7 | |
| 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. | |