SDO HMI 2011-07-20 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 119.34 | 420.47 | 67.15 | 236.69 | -22.59 | 136.33 | 7.19 | 194.05 | 0.4770 | -198.9 | -174.1 | |
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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 | 1.72 | 0.00 | 0.96 | -18.85 | 143.70 | 14.56 | 210.83 | 0.4661 | 665.0 | 526.3 | |
| 0.00 | 4.99 | 0.00 | 2.85 | -22.06 | 142.19 | 13.05 | 204.95 | 0.4980 | 901.0 | 773.1 | |
| 0.00 | 2.54 | 0.00 | 1.45 | -22.46 | 141.95 | 12.81 | 204.20 | 0.5020 | 516.0 | 586.0 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -22.39 | 141.68 | 12.54 | 203.80 | 0.4993 | 768.0 | 701.5 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -22.87 | 141.69 | 12.55 | 203.40 | 0.5059 | 828.0 | 629.0 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.41 | 141.14 | 12.00 | 202.87 | 0.4964 | 838.0 | 650.1 | |
| 0.00 | 4.08 | 0.00 | 2.32 | -22.44 | 140.77 | 11.63 | 202.22 | 0.4947 | 702.0 | 550.0 | |
| 2.27 | 5.17 | 1.29 | 2.94 | -22.50 | 140.31 | 11.16 | 201.37 | 0.4929 | 950.7 | 770.7 | |
| 0.00 | 3.72 | 0.00 | 2.14 | -23.81 | 140.21 | 11.07 | 200.21 | 0.5107 | 513.0 | 560.9 | |
| 2.18 | 3.09 | 1.24 | 1.75 | -22.63 | 139.91 | 10.77 | 200.59 | 0.4926 | 748.8 | 768.6 | |
| 0.00 | 5.72 | 0.00 | 3.28 | -23.46 | 139.91 | 10.77 | 199.96 | 0.5042 | 760.0 | 646.3 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -23.87 | 139.88 | 10.74 | 199.60 | 0.5099 | 744.0 | 687.2 | |
| 17.33 | 40.57 | 9.81 | 22.93 | -22.22 | 139.71 | 10.57 | 200.56 | 0.4856 | 1029.9 | 749.9 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -24.29 | 139.85 | 10.71 | 199.25 | 0.5156 | 561.0 | 458.7 | |
| 3.36 | 4.36 | 1.91 | 2.48 | -22.87 | 139.56 | 10.42 | 199.80 | 0.4940 | 805.4 | 785.1 | |
| 2.54 | 11.71 | 1.45 | 6.67 | -23.00 | 139.27 | 10.13 | 199.19 | 0.4945 | 937.7 | 550.5 | |
| 3.18 | -13.00 | 1.79 | -13.00 | -21.90 | 139.15 | 10.01 | 199.80 | 0.4782 | 991.8 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -23.76 | 139.16 | 10.02 | 198.46 | 0.5047 | 624.0 | 559.9 | |
| 1.27 | -16.00 | 0.72 | -16.00 | -23.06 | 139.07 | 9.93 | 198.80 | 0.4944 | 762.4 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -22.20 | 138.81 | 9.67 | 198.95 | 0.4808 | 568.0 | 511.4 | |
| 0.00 | 3.27 | 0.00 | 1.87 | -23.54 | 138.80 | 9.66 | 198.00 | 0.5000 | 816.0 | 637.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -20.67 | 138.61 | 9.47 | 199.74 | 0.4576 | 896.0 | 638.2 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -22.10 | 138.63 | 9.49 | 198.71 | 0.4784 | 730.0 | 646.6 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -20.84 | 138.52 | 9.38 | 199.43 | 0.4595 | 819.0 | 692.8 | |
| 0.00 | 1.63 | 0.00 | 0.92 | -21.92 | 138.42 | 9.28 | 198.44 | 0.4748 | 881.0 | 690.6 | |
| 0.00 | 4.36 | 0.00 | 2.47 | -22.85 | 138.35 | 9.21 | 197.67 | 0.4879 | 551.0 | 532.7 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -21.99 | 138.26 | 9.12 | 198.10 | 0.4750 | 871.0 | 773.2 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -22.84 | 138.02 | 8.88 | 197.07 | 0.4863 | 841.0 | 644.8 | |
| 5.72 | 7.17 | 3.21 | 4.03 | -22.05 | 137.80 | 8.66 | 197.20 | 0.4738 | 820.0 | 629.9 | |
| 0.36 | 2.09 | 0.21 | 1.18 | -22.80 | 137.75 | 8.61 | 196.61 | 0.4845 | 736.5 | 564.8 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -22.07 | 136.64 | 7.50 | 195.00 | 0.4691 | 33.0 | 43.1 | |
| 0.00 | 15.88 | 0.00 | 8.88 | -21.93 | 136.40 | 7.26 | 194.62 | 0.4661 | -303.0 | -319.2 | |
| 1.63 | 204.01 | 0.92 | 114.34 | -22.86 | 136.35 | 7.21 | 194.00 | 0.4796 | -428.8 | -506.4 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -23.34 | 136.14 | 7.00 | 193.36 | 0.4860 | -625.0 | -402.9 | |
| 1.18 | -33.00 | 0.67 | -33.00 | -22.89 | 136.08 | 6.94 | 193.49 | 0.4791 | -517.8 | 999999 | |
| 7.26 | -33.00 | 4.08 | -33.00 | -22.71 | 135.77 | 6.63 | 193.00 | 0.4754 | -861.3 | 999999 | |
| 7.44 | -33.00 | 4.15 | -33.00 | -21.89 | 135.57 | 6.43 | 193.04 | 0.4624 | -974.4 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -23.89 | 135.56 | 6.42 | 192.04 | 0.4922 | -647.0 | -458.5 | |
| 26.86 | -33.00 | 15.07 | -33.00 | -22.50 | 135.23 | 6.09 | 192.08 | 0.4705 | -1138.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.16 | 134.97 | 5.83 | 190.85 | 0.4945 | -781.0 | -548.5 | |
| 3.09 | 3.81 | 1.74 | 2.16 | -23.46 | 134.88 | 5.73 | 190.97 | 0.4838 | -803.2 | -587.9 | |
| 15.88 | -33.00 | 8.90 | -33.00 | -22.53 | 134.70 | 5.56 | 191.04 | 0.4693 | -1088.1 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -24.09 | 134.74 | 5.59 | 190.45 | 0.4928 | -960.0 | -735.7 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -24.02 | 134.53 | 5.39 | 190.10 | 0.4912 | -473.0 | -477.3 | |
| 0.00 | 3.54 | 0.00 | 2.02 | -24.40 | 134.45 | 5.31 | 189.80 | 0.4967 | -784.0 | -733.9 | |
| 0.00 | 1.82 | 0.00 | 1.03 | -24.12 | 134.30 | 5.16 | 189.64 | 0.4921 | -729.0 | -694.0 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -24.36 | 134.21 | 5.07 | 189.39 | 0.4955 | -647.0 | -563.3 | |
| 15.97 | 56.27 | 8.97 | 31.57 | -22.87 | 134.02 | 4.88 | 189.59 | 0.4725 | -1074.2 | -435.0 | |
| 1.82 | -48.00 | 1.02 | -48.00 | -22.66 | 133.58 | 4.44 | 188.81 | 0.4682 | -908.8 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -24.35 | 132.80 | 3.66 | 186.81 | 0.4924 | -742.0 | -490.1 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -24.56 | 132.34 | 3.20 | 185.91 | 0.4947 | -879.0 | -716.9 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -24.00 | 131.92 | 2.78 | 185.26 | 0.4856 | -827.0 | -713.1 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -24.70 | 131.64 | 2.49 | 184.59 | 0.4958 | -800.0 | -650.6 | |
| 0.00 | 2.27 | 0.00 | 1.29 | -24.28 | 131.59 | 2.45 | 184.59 | 0.4894 | -843.0 | -706.3 | |
| 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. | |