SDO HMI 2014-07-11 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.13 | 231.12 | 23.19 | 145.68 | -19.96 | 147.87 | -30.04 | 130.24 | 0.6176 | 322.1 | 12.9 | |
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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 | -18.96 | 163.84 | -14.07 | 149.33 | 0.4527 | 666.0 | 469.7 | |
| 0.00 | 2.09 | 0.00 | 1.11 | -8.37 | 160.33 | -17.58 | 125.17 | 0.3672 | 740.0 | 550.0 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -22.14 | 157.35 | -20.56 | 143.28 | 0.5463 | 618.0 | 559.3 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -14.17 | 155.25 | -22.66 | 129.35 | 0.4850 | 577.0 | 480.0 | |
| 0.00 | 1.91 | 0.00 | 1.15 | -21.54 | 153.43 | -24.48 | 137.79 | 0.5759 | 784.0 | 550.1 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -21.52 | 153.07 | -24.84 | 137.37 | 0.5791 | 562.0 | 505.6 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -22.83 | 152.27 | -25.64 | 138.11 | 0.5995 | 482.0 | 391.6 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -19.93 | 152.49 | -25.42 | 134.67 | 0.5695 | 687.0 | 602.8 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -17.69 | 152.25 | -25.66 | 131.32 | 0.5514 | 720.0 | 586.4 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -19.71 | 151.88 | -26.03 | 133.73 | 0.5738 | 248.0 | 318.2 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -17.46 | 152.08 | -25.83 | 130.81 | 0.5513 | 663.0 | 488.8 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -17.31 | 151.64 | -26.27 | 130.14 | 0.5549 | 699.0 | 451.6 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -12.02 | 151.35 | -26.56 | 121.55 | 0.5152 | 696.0 | 617.8 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -19.54 | 149.84 | -28.07 | 131.44 | 0.5937 | 742.0 | 699.6 | |
| 10.44 | 64.81 | 6.46 | 40.31 | -20.12 | 149.62 | -28.29 | 131.98 | 0.6009 | 933.6 | 210.3 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -20.70 | 149.31 | -28.60 | 132.45 | 0.6090 | 95.0 | 123.8 | |
| 1.82 | -15.00 | 1.13 | -15.00 | -20.43 | 149.26 | -28.65 | 132.05 | 0.6073 | 600.5 | 999999 | |
| 4.54 | -15.00 | 2.81 | -15.00 | -19.93 | 149.32 | -28.59 | 131.45 | 0.6024 | 1029.4 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.73 | -19.49 | 149.37 | -28.54 | 130.92 | 0.5982 | 851.0 | 720.8 | |
| 0.00 | 1.18 | 0.00 | 0.73 | -19.66 | 149.30 | -28.61 | 131.08 | 0.6003 | 904.0 | 770.5 | |
| 10.53 | -15.00 | 6.55 | -15.00 | -20.07 | 149.07 | -28.84 | 131.40 | 0.6062 | 782.3 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.06 | -18.90 | 149.27 | -28.64 | 130.02 | 0.5944 | 770.0 | 650.1 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -15.94 | 149.77 | -28.14 | 126.28 | 0.5646 | 793.0 | 709.4 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -15.92 | 149.38 | -28.53 | 125.89 | 0.5691 | 556.0 | 462.2 | |
| 0.00 | 1.00 | 0.00 | 0.63 | -21.17 | 148.20 | -29.71 | 132.02 | 0.6243 | 254.0 | 207.5 | |
| 0.00 | 1.82 | 0.00 | 1.16 | -21.92 | 147.92 | -29.99 | 132.72 | 0.6334 | 640.0 | 515.0 | |
| 0.00 | 0.64 | 0.00 | 0.40 | -19.73 | 148.36 | -29.55 | 130.29 | 0.6108 | 616.0 | 516.0 | |
| 1.27 | 2.45 | 0.80 | 1.53 | -19.86 | 148.26 | -29.65 | 130.38 | 0.6130 | 813.2 | 678.0 | |
| 0.00 | 0.73 | 0.00 | 0.43 | -13.39 | 149.24 | -28.67 | 121.88 | 0.5517 | 732.0 | 647.4 | |
| 1.54 | 38.03 | 0.97 | 24.03 | -20.27 | 148.02 | -29.89 | 130.70 | 0.6188 | 676.6 | 76.3 | |
| 1.00 | 2.63 | 0.64 | 1.68 | -21.52 | 147.74 | -30.17 | 132.06 | 0.6319 | 572.8 | 434.1 | |
| 0.00 | 2.54 | 0.00 | 1.59 | -19.87 | 148.00 | -29.91 | 130.15 | 0.6159 | 657.0 | 538.1 | |
| 0.00 | 0.91 | 0.00 | 0.55 | -15.52 | 148.79 | -29.12 | 124.76 | 0.5729 | 627.0 | 481.2 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -19.62 | 147.52 | -30.39 | 129.40 | 0.6189 | 632.0 | 498.3 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -18.80 | 147.47 | -30.44 | 128.25 | 0.6130 | 698.0 | 504.6 | |
| 0.00 | 3.63 | 0.00 | 2.28 | -19.04 | 147.19 | -30.72 | 128.34 | 0.6178 | 718.0 | 572.6 | |
| 1.18 | 53.73 | 0.75 | 34.37 | -19.75 | 146.93 | -30.98 | 129.05 | 0.6261 | 651.6 | -194.6 | |
| 0.00 | 2.45 | 0.00 | 1.57 | -20.40 | 146.33 | -31.58 | 129.40 | 0.6375 | -401.0 | -402.8 | |
| 2.45 | -37.00 | 1.56 | -37.00 | -19.70 | 146.37 | -31.54 | 128.52 | 0.6316 | 505.7 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.88 | -20.65 | 146.00 | -31.91 | 129.44 | 0.6427 | -717.0 | -622.1 | |
| 0.00 | 2.54 | 0.00 | 1.65 | -20.89 | 145.83 | -32.08 | 129.61 | 0.6463 | -672.0 | -640.5 | |
| 0.00 | 1.27 | 0.00 | 0.82 | -20.42 | 145.90 | -32.01 | 129.06 | 0.6420 | -696.0 | -567.5 | |
| 0.00 | 1.36 | 0.00 | 0.89 | -21.23 | 145.67 | -32.24 | 129.91 | 0.6506 | -602.0 | -543.3 | |
| 2.36 | -37.00 | 1.52 | -37.00 | -19.82 | 145.69 | -32.22 | 128.12 | 0.6397 | -445.3 | 999999 | |
| 0.00 | 2.18 | 0.00 | 1.42 | -20.72 | 144.86 | -33.05 | 128.62 | 0.6551 | -773.0 | -628.8 | |
| 0.00 | 3.63 | 0.00 | 2.39 | -21.10 | 144.69 | -33.22 | 128.96 | 0.6596 | -611.0 | -546.9 | |
| 0.00 | 1.36 | 0.00 | 0.89 | -20.53 | 144.79 | -33.12 | 128.31 | 0.6543 | -773.0 | -626.1 | |
| 0.00 | 0.91 | 0.00 | 0.60 | -21.71 | 144.45 | -33.46 | 129.54 | 0.6665 | -601.0 | -518.9 | |
| 0.00 | 2.18 | 0.00 | 1.43 | -20.90 | 144.58 | -33.33 | 128.62 | 0.6592 | -892.0 | -762.0 | |
| 0.00 | 2.09 | 0.00 | 1.39 | -22.07 | 144.04 | -33.87 | 129.66 | 0.6732 | -640.0 | -546.0 | |
| 0.00 | 1.09 | 0.00 | 0.72 | -20.95 | 144.22 | -33.69 | 128.40 | 0.6633 | -781.0 | -678.9 | |
| 0.00 | 1.09 | 0.00 | 0.73 | -21.49 | 143.28 | -34.63 | 128.37 | 0.6767 | -657.0 | -610.1 | |
| 0.00 | 1.00 | 0.00 | 0.67 | -21.70 | 143.18 | -34.73 | 128.55 | 0.6791 | -597.0 | -502.1 | |
| 0.00 | 1.00 | 0.00 | 0.68 | -22.46 | 142.76 | -35.15 | 129.18 | 0.6885 | -674.0 | -535.6 | |
| 0.00 | 2.09 | 0.00 | 1.40 | -21.27 | 142.90 | -35.01 | 127.81 | 0.6790 | -551.0 | -465.7 | |
| 0.00 | 1.45 | 0.00 | 0.99 | -22.47 | 142.52 | -35.39 | 129.01 | 0.6910 | -547.0 | -469.1 | |
| 0.00 | 1.63 | 0.00 | 1.07 | -18.90 | 143.20 | -34.71 | 124.98 | 0.6599 | -728.0 | -569.4 | |
| 0.00 | 1.72 | 0.00 | 1.17 | -20.99 | 142.34 | -35.57 | 127.05 | 0.6828 | -582.0 | -433.6 | |
| 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. | |