SDO HMI 2011-06-20 18:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 120.00 | 657.22 | 62.21 | 340.70 | 17.14 | 168.43 | 6.66 | 338.01 | 0.2952 | -461.8 | -254.4 | |
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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 | 1.81 | 0.00 | 0.96 | 15.41 | 177.45 | 15.69 | 312.53 | 0.3552 | -721.0 | -631.3 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 11.31 | 176.44 | 14.68 | 304.22 | 0.3017 | -716.0 | -525.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 11.31 | 176.15 | 14.39 | 304.74 | 0.2978 | -935.0 | -779.6 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 13.34 | 174.46 | 12.70 | 313.57 | 0.2965 | -739.0 | -534.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 12.69 | 174.33 | 12.57 | 312.17 | 0.2877 | -645.0 | -495.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 13.34 | 173.95 | 12.19 | 314.73 | 0.2904 | -817.0 | -665.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 13.47 | 173.83 | 12.06 | 315.33 | 0.2904 | -813.0 | -579.2 | |
| 0.00 | 2.18 | 0.00 | 1.13 | 13.47 | 173.61 | 11.84 | 315.86 | 0.2878 | -790.0 | -663.8 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 12.66 | 173.31 | 11.55 | 314.48 | 0.2749 | -806.0 | -666.3 | |
| 0.00 | 3.90 | 0.00 | 2.00 | 12.08 | 172.46 | 10.69 | 315.04 | 0.2579 | -690.0 | -629.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.42 | 172.41 | 10.65 | 325.26 | 0.3124 | 892.0 | 767.2 | |
| 1.27 | 2.27 | 0.66 | 1.17 | 15.57 | 171.60 | 9.83 | 325.71 | 0.2932 | 803.9 | 458.9 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.49 | 171.32 | 9.55 | 328.20 | 0.3033 | -774.0 | -556.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 20.05 | 171.45 | 9.69 | 333.43 | 0.3550 | -726.0 | -549.2 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 19.86 | 171.28 | 9.51 | 333.59 | 0.3510 | -664.0 | -584.1 | |
| 93.97 | 506.29 | 48.83 | 263.10 | 17.38 | 169.65 | 7.89 | 334.25 | 0.3028 | -1573.1 | -443.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 14.08 | 169.53 | 7.76 | 328.73 | 0.2535 | -847.0 | -602.2 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 13.62 | 169.00 | 7.24 | 329.48 | 0.2422 | -864.0 | -689.6 | |
| 1.00 | -16.00 | 0.52 | -16.00 | 17.89 | 169.03 | 7.26 | 336.74 | 0.3061 | -896.9 | 999999 | |
| 0.00 | 2.27 | 0.00 | 1.17 | 17.42 | 168.11 | 6.35 | 338.81 | 0.2930 | -70.0 | -82.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 14.21 | 166.97 | 5.20 | 338.02 | 0.2359 | -714.0 | -514.4 | |
| 0.00 | 4.26 | 0.00 | 2.17 | 14.68 | 165.97 | 4.20 | 342.56 | 0.2377 | -995.0 | -832.8 | |
| 0.00 | 2.36 | 0.00 | 1.22 | 17.64 | 165.39 | 3.63 | 347.67 | 0.2835 | 638.0 | 552.3 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.25 | 164.67 | 2.90 | 350.46 | 0.2911 | 776.0 | 669.4 | |
| 0.00 | 2.36 | 0.00 | 1.21 | 17.08 | 164.62 | 2.85 | 349.88 | 0.2716 | 895.0 | 778.2 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 17.27 | 164.40 | 2.63 | 350.76 | 0.2741 | 1082.0 | 834.2 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 17.33 | 164.08 | 2.31 | 351.90 | 0.2744 | 897.0 | 820.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 13.53 | 164.00 | 2.24 | 349.56 | 0.2105 | 820.0 | 559.1 | |
| 0.00 | 2.90 | 0.00 | 1.49 | 16.79 | 163.75 | 1.99 | 352.77 | 0.2647 | 885.0 | 773.5 | |
| 0.00 | 6.62 | 0.00 | 3.40 | 16.67 | 163.53 | 1.76 | 353.52 | 0.2621 | 1220.0 | 922.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 15.06 | 163.48 | 1.72 | 352.90 | 0.2350 | -908.0 | -667.3 | |
| 0.00 | 4.63 | 0.00 | 2.39 | 17.87 | 163.28 | 1.52 | 354.85 | 0.2818 | 797.0 | 902.6 | |
| 4.44 | 47.07 | 2.27 | 24.07 | 16.07 | 163.21 | 1.44 | 354.47 | 0.2515 | 1062.5 | 641.4 | |
| 0.00 | 4.17 | 0.00 | 2.16 | 18.22 | 163.19 | 1.42 | 355.27 | 0.2876 | 959.0 | 780.7 | |
| 11.25 | -33.00 | 5.75 | -33.00 | 16.07 | 162.86 | 1.09 | 355.80 | 0.2510 | 1169.4 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 18.00 | 162.87 | 1.10 | 356.28 | 0.2834 | 692.0 | 535.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 16.79 | 161.33 | -0.43 | 1.58 | 0.2627 | 895.0 | 746.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.81 | 161.15 | -0.62 | 2.61 | 0.2292 | 825.0 | 576.6 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 15.88 | 161.08 | -0.68 | 2.67 | 0.2473 | 1050.0 | 802.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 15.57 | 161.08 | -0.68 | 2.73 | 0.2420 | 849.0 | 518.5 | |
| 8.07 | 8.98 | 4.18 | 4.65 | 18.34 | 161.01 | -0.76 | 2.50 | 0.2890 | 1022.8 | 712.8 | |
| 0.00 | 2.18 | 0.00 | 1.14 | 21.07 | 160.83 | -0.93 | 2.61 | 0.3344 | 804.0 | 579.7 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 17.49 | 160.47 | -1.30 | 4.51 | 0.2752 | 983.0 | 856.7 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 17.08 | 160.38 | -1.39 | 4.97 | 0.2684 | 861.0 | 744.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.87 | 160.08 | -1.68 | 5.71 | 0.2821 | 943.0 | 786.2 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.96 | 160.08 | -1.68 | 5.68 | 0.2837 | 667.0 | 635.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 17.14 | 160.06 | -1.71 | 6.08 | 0.2699 | 855.0 | 633.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.65 | 159.99 | -1.78 | 6.11 | 0.2786 | 927.0 | 745.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 19.97 | 159.90 | -1.87 | 5.56 | 0.3174 | 845.0 | 662.4 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 18.31 | 159.82 | -1.94 | 6.40 | 0.2900 | 968.0 | 892.2 | |
| 0.00 | 2.81 | 0.00 | 1.45 | 17.71 | 159.77 | -2.00 | 6.85 | 0.2800 | 1091.0 | 828.6 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.60 | 159.72 | -2.04 | 6.61 | 0.2949 | 883.0 | 714.4 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 20.49 | 159.63 | -2.13 | 6.16 | 0.3264 | 764.0 | 647.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 18.15 | 159.34 | -2.42 | 8.04 | 0.2883 | 844.0 | 659.9 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 14.18 | 157.25 | -4.51 | 19.35 | 0.2313 | -782.0 | -595.7 | |
| 0.00 | 3.08 | 0.00 | 1.57 | 14.52 | 156.05 | -5.72 | 23.39 | 0.2442 | 928.0 | 847.5 | |
| 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. | |