SDO HMI 2011-06-20 16:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 118.27 | 670.59 | 61.19 | 346.95 | 17.25 | 168.30 | 5.42 | 341.91 | 0.2896 | -425.2 | -245.7 | |
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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 | 0.73 | 0.00 | 0.37 | 13.25 | 174.35 | 11.48 | 316.19 | 0.2810 | -844.0 | -659.1 | |
| 0.00 | 2.54 | 0.00 | 1.31 | 13.31 | 174.17 | 11.29 | 316.82 | 0.2796 | -859.0 | -749.7 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 14.03 | 173.59 | 10.72 | 320.03 | 0.2820 | -739.0 | -457.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 12.69 | 173.31 | 10.43 | 317.43 | 0.2623 | -968.0 | -765.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.42 | 172.36 | 9.48 | 328.26 | 0.3018 | 999.0 | 800.3 | |
| 1.45 | 3.45 | 0.75 | 1.78 | 15.57 | 171.58 | 8.71 | 328.84 | 0.2831 | 868.5 | 324.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.55 | 171.27 | 8.40 | 331.49 | 0.2946 | -898.0 | -629.2 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 16.30 | 171.10 | 8.23 | 331.55 | 0.2895 | -861.0 | -610.2 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 16.14 | 170.90 | 8.03 | 331.86 | 0.2857 | -669.0 | -527.8 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.02 | 170.71 | 7.83 | 332.23 | 0.2823 | -817.0 | -479.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 13.05 | 170.13 | 7.25 | 328.18 | 0.2343 | -653.0 | -670.2 | |
| 56.87 | 516.20 | 29.52 | 267.61 | 17.66 | 169.71 | 6.84 | 337.68 | 0.3000 | -1498.0 | -449.4 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 14.11 | 169.53 | 6.65 | 332.54 | 0.2448 | -851.0 | -661.2 | |
| 32.38 | -12.00 | 16.75 | -12.00 | 17.03 | 169.53 | 6.65 | 337.37 | 0.2891 | -1701.4 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 13.71 | 168.95 | 6.07 | 333.85 | 0.2342 | -1016.0 | -781.9 | |
| 1.18 | -12.00 | 0.61 | -12.00 | 17.92 | 168.95 | 6.07 | 340.26 | 0.2994 | -838.6 | 999999 | |
| 0.00 | 2.18 | 0.00 | 1.11 | 14.27 | 167.86 | 4.98 | 338.96 | 0.2356 | -965.0 | -782.2 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 13.71 | 167.72 | 4.85 | 338.59 | 0.2258 | -819.0 | -685.3 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.40 | 167.50 | 4.62 | 343.14 | 0.2677 | 646.0 | 454.1 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 14.33 | 167.20 | 4.32 | 341.63 | 0.2328 | -951.0 | -753.5 | |
| 0.00 | 2.27 | 0.00 | 1.16 | 16.50 | 165.62 | 2.75 | 349.85 | 0.2619 | 806.0 | 639.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.64 | 165.38 | 2.51 | 351.41 | 0.2801 | 585.0 | 553.4 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.24 | 164.65 | 1.78 | 354.12 | 0.2886 | 805.0 | 591.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.96 | 164.62 | 1.74 | 354.13 | 0.2838 | 793.0 | 619.6 | |
| 0.00 | 7.17 | 0.00 | 3.69 | 17.16 | 164.52 | 1.64 | 354.17 | 0.2704 | 995.0 | 693.9 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 17.73 | 164.26 | 1.39 | 355.25 | 0.2795 | 846.0 | 697.0 | |
| 0.00 | 3.81 | 0.00 | 1.97 | 18.37 | 164.11 | 1.23 | 355.95 | 0.2900 | 819.0 | 620.0 | |
| 0.00 | 3.45 | 0.00 | 1.77 | 17.39 | 164.07 | 1.19 | 355.81 | 0.2734 | 1001.0 | 827.2 | |
| 0.36 | 2.54 | 0.19 | 1.30 | 16.82 | 163.75 | 0.87 | 356.82 | 0.2635 | 1041.5 | 832.9 | |
| 2.45 | 6.17 | 1.26 | 3.16 | 16.60 | 163.56 | 0.68 | 357.48 | 0.2596 | 988.7 | 969.9 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.09 | 163.49 | 0.61 | 357.46 | 0.2340 | -956.0 | -818.1 | |
| 0.00 | 4.99 | 0.00 | 2.57 | 17.89 | 163.24 | 0.36 | 358.76 | 0.2813 | 1011.0 | 870.5 | |
| 3.81 | 47.44 | 1.95 | 24.25 | 16.06 | 163.21 | 0.33 | 358.73 | 0.2504 | 1094.2 | 654.2 | |
| 0.00 | 7.26 | 0.00 | 3.75 | 18.18 | 163.18 | 0.30 | 358.99 | 0.2861 | 917.0 | 741.5 | |
| 1.54 | -33.00 | 0.79 | -33.00 | 15.87 | 163.08 | 0.20 | 359.21 | 0.2471 | 1163.0 | 999999 | |
| 5.44 | -33.00 | 2.79 | -33.00 | 16.19 | 162.89 | 0.01 | 359.95 | 0.2524 | 1007.8 | 999999 | |
| 3.63 | -33.00 | 1.85 | -33.00 | 15.94 | 162.86 | -0.02 | 0.07 | 0.2482 | 1330.0 | 999999 | |
| 0.91 | -33.00 | 0.46 | -33.00 | 15.97 | 162.64 | -0.24 | 0.93 | 0.2487 | 1051.7 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 19.94 | 161.72 | -1.15 | 3.45 | 0.3160 | 846.0 | 661.0 | |
| 8.25 | 10.98 | 4.27 | 5.68 | 18.31 | 161.06 | -1.82 | 5.98 | 0.2898 | 1003.1 | 355.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 17.51 | 160.49 | -2.38 | 8.24 | 0.2777 | 853.0 | 724.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 17.01 | 160.31 | -2.57 | 9.18 | 0.2698 | 995.0 | 852.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 17.64 | 160.27 | -2.61 | 8.94 | 0.2804 | 793.0 | 584.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.83 | 160.14 | -2.74 | 9.26 | 0.2839 | 970.0 | 797.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.64 | 159.98 | -2.90 | 9.90 | 0.2812 | 942.0 | 764.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.24 | 159.84 | -3.03 | 9.97 | 0.2915 | 971.0 | 833.2 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 20.03 | 159.81 | -3.07 | 9.05 | 0.3210 | 822.0 | 642.2 | |
| 0.00 | 2.99 | 0.00 | 1.55 | 17.76 | 159.79 | -3.09 | 10.47 | 0.2838 | 969.0 | 884.4 | |
| 0.00 | 2.81 | 0.00 | 1.45 | 17.92 | 159.46 | -3.41 | 11.42 | 0.2875 | 814.0 | 717.4 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.49 | 159.45 | -3.42 | 11.05 | 0.2969 | 654.0 | 524.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.24 | 159.30 | -3.58 | 11.72 | 0.2932 | 778.0 | 591.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.59 | 158.66 | -4.22 | 15.26 | 0.2689 | 867.0 | 665.8 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.72 | 158.02 | -4.86 | 17.30 | 0.2739 | 602.0 | 512.0 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 14.17 | 157.26 | -5.62 | 23.60 | 0.2382 | -643.0 | -464.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 14.42 | 156.05 | -6.83 | 27.46 | 0.2508 | 994.0 | 868.6 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 14.86 | 155.94 | -6.93 | 27.01 | 0.2582 | 787.0 | 667.2 | |
| 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. | |