SDO HMI 2011-07-19 21:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.37 | 319.80 | 44.13 | 178.45 | -22.51 | 136.55 | 0.27 | 180.56 | 0.4611 | -107.0 | -165.2 | |
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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 | 1.09 | 0.00 | 0.60 | -21.05 | 142.71 | 6.43 | 193.53 | 0.4488 | 789.0 | 573.8 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -22.17 | 142.14 | 5.85 | 191.80 | 0.4638 | 760.0 | 627.8 | |
| 0.00 | 4.17 | 0.00 | 2.33 | -22.26 | 141.74 | 5.46 | 190.98 | 0.4641 | 759.0 | 700.8 | |
| 0.00 | 3.27 | 0.00 | 1.84 | -23.02 | 141.77 | 5.49 | 190.71 | 0.4757 | 529.0 | 658.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -22.43 | 141.09 | 4.81 | 189.63 | 0.4648 | 741.0 | 525.7 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.54 | 140.69 | 4.41 | 188.15 | 0.4959 | 653.0 | 514.8 | |
| 5.80 | 9.98 | 3.24 | 5.57 | -22.39 | 140.13 | 3.85 | 187.75 | 0.4620 | 987.2 | 855.8 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -23.98 | 140.11 | 3.83 | 187.23 | 0.4862 | 700.0 | 572.7 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -22.05 | 139.89 | 3.61 | 187.37 | 0.4562 | 988.0 | 902.7 | |
| 0.00 | 2.99 | 0.00 | 1.69 | -23.70 | 139.87 | 3.58 | 186.86 | 0.4815 | 991.0 | 760.5 | |
| 0.82 | 29.02 | 0.45 | 16.19 | -22.28 | 139.66 | 3.38 | 186.85 | 0.4594 | 1133.6 | 808.6 | |
| 1.36 | -11.00 | 0.76 | -11.00 | -22.46 | 139.67 | 3.39 | 186.81 | 0.4621 | 780.9 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.18 | -23.70 | 139.60 | 3.32 | 186.35 | 0.4810 | 760.0 | 535.3 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -24.57 | 139.52 | 3.24 | 185.99 | 0.4941 | 606.0 | 453.6 | |
| 4.90 | -11.00 | 2.73 | -11.00 | -22.18 | 139.40 | 3.12 | 186.34 | 0.4573 | 1181.4 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.12 | -22.69 | 139.18 | 2.90 | 185.78 | 0.4649 | 802.0 | 643.2 | |
| 2.54 | -11.00 | 1.41 | -11.00 | -22.32 | 139.14 | 2.85 | 185.78 | 0.4590 | 866.5 | 999999 | |
| 9.80 | 13.15 | 5.42 | 7.28 | -21.60 | 139.09 | 2.81 | 185.86 | 0.4478 | 1081.9 | 735.2 | |
| 0.00 | 2.18 | 0.00 | 1.23 | -23.69 | 139.10 | 2.82 | 185.40 | 0.4802 | 804.0 | 684.5 | |
| 0.00 | 2.45 | 0.00 | 1.38 | -23.35 | 138.93 | 2.64 | 185.14 | 0.4746 | 545.0 | 538.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -20.11 | 138.83 | 2.55 | 185.68 | 0.4241 | 713.0 | 663.2 | |
| 0.00 | 1.81 | 0.00 | 1.02 | -23.04 | 138.82 | 2.54 | 185.00 | 0.4697 | 740.0 | 591.7 | |
| 0.00 | 3.99 | 0.00 | 2.22 | -22.32 | 138.74 | 2.46 | 184.99 | 0.4584 | 830.0 | 640.5 | |
| 0.00 | 4.35 | 0.00 | 2.42 | -22.07 | 138.41 | 2.13 | 184.36 | 0.4543 | 884.0 | 724.0 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -22.55 | 138.35 | 2.07 | 184.16 | 0.4616 | 441.0 | 362.4 | |
| 0.00 | 2.99 | 0.00 | 1.67 | -22.76 | 138.12 | 1.84 | 183.67 | 0.4646 | 525.0 | 493.1 | |
| 1.09 | 1.72 | 0.60 | 0.95 | -21.70 | 137.98 | 1.69 | 183.53 | 0.4479 | 504.5 | 502.1 | |
| 0.00 | 2.72 | 0.00 | 1.55 | -24.84 | 137.75 | 1.47 | 182.69 | 0.4962 | 390.0 | 481.4 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -24.14 | 137.47 | 1.19 | 182.25 | 0.4853 | 357.0 | 408.7 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -21.76 | 137.06 | 0.78 | 181.61 | 0.4483 | 418.0 | 343.1 | |
| 0.00 | 11.88 | 0.00 | 6.63 | -22.58 | 136.83 | 0.55 | 181.11 | 0.4610 | -463.0 | -325.9 | |
| 4.08 | 183.03 | 2.26 | 101.87 | -21.73 | 136.50 | 0.22 | 180.46 | 0.4476 | -998.9 | -557.4 | |
| 2.09 | -32.00 | 1.16 | -32.00 | -22.58 | 136.30 | 0.02 | 180.04 | 0.4610 | -601.9 | 999999 | |
| 4.81 | -32.00 | 2.66 | -32.00 | -21.87 | 136.24 | -0.04 | 179.91 | 0.4497 | -1089.0 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -23.20 | 136.01 | -0.28 | 179.46 | 0.4706 | -644.0 | -513.4 | |
| 8.34 | -32.00 | 4.64 | -32.00 | -22.38 | 135.94 | -0.34 | 179.31 | 0.4578 | -1042.5 | 999999 | |
| 2.18 | -32.00 | 1.21 | -32.00 | -22.00 | 135.74 | -0.54 | 178.89 | 0.4520 | -1038.6 | 999999 | |
| 1.54 | -32.00 | 0.86 | -32.00 | -22.21 | 135.58 | -0.70 | 178.57 | 0.4552 | -995.7 | 999999 | |
| 5.17 | -32.00 | 2.88 | -32.00 | -22.35 | 135.38 | -0.90 | 178.17 | 0.4574 | -1048.1 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -24.04 | 135.30 | -0.98 | 178.14 | 0.4836 | -869.0 | -626.1 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -23.97 | 135.07 | -1.21 | 177.70 | 0.4827 | -813.0 | -596.8 | |
| 7.62 | -32.00 | 4.24 | -32.00 | -22.41 | 135.05 | -1.23 | 177.51 | 0.4587 | -1156.7 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -23.17 | 135.04 | -1.24 | 177.57 | 0.4705 | -538.0 | -377.9 | |
| 0.00 | 4.35 | 0.00 | 2.44 | -22.96 | 134.85 | -1.43 | 177.16 | 0.4674 | -820.0 | -630.0 | |
| 1.36 | -32.00 | 0.76 | -32.00 | -22.24 | 134.82 | -1.46 | 177.03 | 0.4562 | -1016.4 | 999999 | |
| 0.00 | 2.63 | 0.00 | 1.49 | -24.18 | 134.73 | -1.55 | 177.08 | 0.4861 | -944.0 | -844.7 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -24.00 | 134.60 | -1.68 | 176.81 | 0.4836 | -838.0 | -775.0 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -24.35 | 134.50 | -1.78 | 176.66 | 0.4890 | -803.0 | -632.5 | |
| 14.15 | -32.00 | 7.89 | -32.00 | -22.52 | 134.29 | -1.99 | 175.99 | 0.4610 | -1140.8 | 999999 | |
| 1.72 | -32.00 | 0.96 | -32.00 | -22.35 | 133.96 | -2.32 | 175.31 | 0.4588 | -1045.4 | 999999 | |
| 0.00 | 4.35 | 0.00 | 2.48 | -24.53 | 133.62 | -2.66 | 175.07 | 0.4927 | -667.0 | -572.8 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.64 | 132.51 | -3.77 | 173.06 | 0.4961 | -613.0 | -499.4 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -25.87 | 132.44 | -3.84 | 173.25 | 0.5147 | -623.0 | -522.1 | |
| 0.00 | 2.72 | 0.00 | 1.55 | -24.72 | 131.74 | -4.54 | 171.67 | 0.4988 | -852.0 | -675.3 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -23.76 | 128.96 | -7.32 | 166.25 | 0.4927 | 429.0 | 463.5 | |
| 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. | |