SDO HMI 2011-10-26 15:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.27 | 148.10 | 9.82 | 75.75 | 16.34 | 279.10 | 7.05 | 330.71 | 0.2429 | -27.4 | -52.4 | |
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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 | 0.61 | 0.00 | 0.32 | 13.00 | 290.84 | 18.80 | 294.76 | 0.3473 | -737.0 | -641.6 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 13.43 | 290.85 | 18.80 | 295.88 | 0.3500 | -860.0 | -697.0 | |
| 0.00 | 1.74 | 0.00 | 0.91 | 12.83 | 290.51 | 18.46 | 294.65 | 0.3413 | -914.0 | -754.8 | |
| 0.00 | 1.30 | 0.00 | 0.69 | 15.37 | 290.36 | 18.32 | 301.45 | 0.3568 | -740.0 | -556.2 | |
| 0.00 | 3.30 | 0.00 | 1.75 | 16.76 | 289.55 | 17.51 | 305.93 | 0.3573 | -882.0 | -673.3 | |
| 0.00 | 2.95 | 0.00 | 1.55 | 14.17 | 288.91 | 16.86 | 300.25 | 0.3270 | -728.0 | -591.3 | |
| 0.00 | 2.34 | 0.00 | 1.23 | 14.18 | 288.62 | 16.57 | 300.67 | 0.3230 | -827.0 | -703.4 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 14.72 | 286.01 | 13.96 | 306.44 | 0.2914 | -756.0 | -605.1 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 14.66 | 285.75 | 13.71 | 306.77 | 0.2875 | -696.0 | -668.5 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 21.48 | 284.73 | 12.68 | 324.53 | 0.3536 | 864.0 | 669.4 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 11.66 | 283.59 | 11.54 | 301.22 | 0.2302 | -947.0 | -687.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 23.68 | 284.37 | 12.33 | 328.83 | 0.3793 | 704.0 | 544.1 | |
| 0.00 | 2.78 | 0.00 | 1.42 | 14.23 | 282.77 | 10.72 | 312.10 | 0.2442 | -946.0 | -671.7 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 17.96 | 280.94 | 8.90 | 326.98 | 0.2712 | -739.0 | -608.6 | |
| 18.66 | 45.65 | 9.51 | 23.28 | 16.05 | 280.22 | 8.18 | 324.78 | 0.2381 | -1234.2 | -536.7 | |
| 0.61 | 2.17 | 0.31 | 1.11 | 16.36 | 279.86 | 7.82 | 326.73 | 0.2389 | -784.9 | -801.2 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 18.35 | 279.69 | 7.65 | 331.50 | 0.2659 | -869.0 | -834.5 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 21.03 | 279.76 | 7.71 | 335.73 | 0.3062 | -751.0 | -591.7 | |
| 0.00 | 1.65 | 0.00 | 0.85 | 18.13 | 279.56 | 7.51 | 331.52 | 0.2617 | -867.0 | -877.2 | |
| 0.00 | 7.98 | 0.00 | 4.05 | 15.10 | 278.88 | 6.83 | 327.01 | 0.2120 | -693.0 | -848.5 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 15.67 | 278.80 | 6.76 | 328.77 | 0.2195 | -759.0 | -560.4 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 14.77 | 278.68 | 6.64 | 326.87 | 0.2055 | -985.0 | -822.9 | |
| 0.00 | 1.65 | 0.00 | 0.83 | 14.17 | 278.23 | 6.19 | 327.00 | 0.1927 | -954.0 | -695.6 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 16.77 | 278.03 | 5.98 | 334.10 | 0.2296 | -620.0 | -519.8 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 13.96 | 277.82 | 5.78 | 328.14 | 0.1860 | -994.0 | -771.5 | |
| 0.00 | 4.34 | 0.00 | 2.21 | 16.90 | 277.62 | 5.58 | 335.86 | 0.2286 | 469.0 | 516.9 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 14.20 | 277.52 | 5.48 | 330.17 | 0.1869 | -697.0 | -535.1 | |
| 0.00 | 3.82 | 0.00 | 1.95 | 17.88 | 276.96 | 4.92 | 340.00 | 0.2398 | 1074.0 | 915.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 16.94 | 276.88 | 4.83 | 338.84 | 0.2243 | 846.0 | 764.4 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 17.64 | 276.61 | 4.57 | 340.98 | 0.2339 | 827.0 | 699.7 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 17.40 | 276.42 | 4.37 | 341.38 | 0.2290 | 954.0 | 742.2 | |
| 0.00 | 3.12 | 0.00 | 1.59 | 16.73 | 276.37 | 4.33 | 340.54 | 0.2179 | 724.0 | 791.4 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 17.86 | 276.30 | 4.26 | 342.46 | 0.2358 | 857.0 | 797.1 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.24 | 276.20 | 4.16 | 340.45 | 0.2092 | 1041.0 | 866.7 | |
| 0.00 | 1.74 | 0.00 | 0.87 | 12.08 | 276.10 | 4.05 | 330.95 | 0.1431 | 960.0 | 752.8 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 18.74 | 276.14 | 4.09 | 344.20 | 0.2494 | 769.0 | 608.5 | |
| 0.00 | 2.00 | 0.00 | 1.01 | 17.28 | 276.04 | 4.00 | 342.72 | 0.2250 | 1132.0 | 909.0 | |
| 0.00 | 2.95 | 0.00 | 1.50 | 16.79 | 275.97 | 3.92 | 342.33 | 0.2168 | 1058.0 | 840.6 | |
| 0.00 | 2.34 | 0.00 | 1.17 | 12.32 | 275.86 | 3.81 | 333.20 | 0.1448 | 875.0 | 660.7 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 18.72 | 275.44 | 3.40 | 346.74 | 0.2460 | 838.0 | 682.8 | |
| 0.00 | 1.30 | 0.00 | 0.65 | 11.96 | 275.24 | 3.20 | 335.97 | 0.1347 | 832.0 | 660.8 | |
| 0.00 | 3.47 | 0.00 | 1.77 | 18.81 | 275.13 | 3.09 | 348.01 | 0.2464 | 922.0 | 779.6 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 11.99 | 274.94 | 2.89 | 338.11 | 0.1331 | 801.0 | 724.4 | |
| 0.00 | 1.13 | 0.00 | 0.56 | 12.17 | 274.76 | 2.71 | 339.84 | 0.1349 | 969.0 | 759.4 | |
| 0.00 | 1.56 | 0.00 | 0.78 | 13.83 | 274.47 | 2.42 | 345.12 | 0.1607 | 792.0 | 625.3 | |
| 0.00 | 1.74 | 0.00 | 0.90 | 21.28 | 274.25 | 2.21 | 352.73 | 0.2850 | 1046.0 | 802.3 | |
| 0.00 | 1.13 | 0.00 | 0.56 | 12.81 | 274.00 | 1.96 | 346.34 | 0.1416 | 898.0 | 686.2 | |
| 0.00 | 2.52 | 0.00 | 1.29 | 19.71 | 273.88 | 1.84 | 353.25 | 0.2579 | 817.0 | 640.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 20.94 | 273.42 | 1.37 | 355.36 | 0.2779 | 712.0 | 560.8 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 13.35 | 271.62 | -0.43 | 2.84 | 0.1472 | 908.0 | 651.3 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 19.09 | 271.32 | -0.72 | 2.79 | 0.2460 | 894.0 | 667.3 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 19.37 | 270.97 | -1.07 | 4.05 | 0.2510 | 878.0 | 590.8 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 16.65 | 270.55 | -1.49 | 7.00 | 0.2054 | 833.0 | 711.6 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 16.92 | 268.90 | -3.14 | 14.18 | 0.2152 | 913.0 | 724.6 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 17.10 | 268.87 | -3.18 | 14.11 | 0.2183 | 830.0 | 617.6 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 23.27 | 267.60 | -4.44 | 12.74 | 0.3242 | 891.0 | 730.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 23.02 | 267.57 | -4.47 | 13.00 | 0.3202 | 995.0 | 721.0 | |
| 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. | |