SDO HMI 2014-07-15 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 79.99 | 0.26 | 46.91 | -20.16 | 149.00 | 20.15 | 217.76 | 0.5349 | 193.0 | 223.5 | |
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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 | 0.45 | 0.00 | 0.31 | -24.24 | 162.18 | 33.32 | 226.99 | 0.6873 | -585.0 | -539.6 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -20.89 | 157.70 | 28.85 | 227.19 | 0.6167 | 557.0 | 436.5 | |
| 0.00 | 1.63 | 0.00 | 1.03 | -21.24 | 157.29 | 28.44 | 226.35 | 0.6157 | 119.0 | 184.3 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -20.22 | 156.90 | 28.05 | 227.28 | 0.6028 | 627.0 | 467.8 | |
| 0.00 | 2.36 | 0.00 | 1.46 | -20.37 | 156.64 | 27.78 | 226.82 | 0.6015 | 575.0 | 492.5 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -20.56 | 156.31 | 27.45 | 226.25 | 0.5998 | 662.0 | 477.9 | |
| 0.00 | 2.27 | 0.00 | 1.39 | -19.92 | 156.11 | 27.26 | 226.88 | 0.5920 | 591.0 | 580.4 | |
| 0.00 | 3.63 | 0.00 | 2.23 | -20.15 | 156.12 | 27.26 | 226.59 | 0.5942 | 669.0 | 666.9 | |
| 0.00 | 1.73 | 0.00 | 1.06 | -20.62 | 156.02 | 27.17 | 225.89 | 0.5974 | 728.0 | 558.0 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -20.09 | 155.30 | 26.45 | 225.83 | 0.5854 | 761.0 | 584.3 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -20.38 | 155.03 | 26.18 | 225.17 | 0.5853 | 760.0 | 612.5 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -19.16 | 154.31 | 25.46 | 226.02 | 0.5665 | 629.0 | 546.6 | |
| 0.00 | 1.45 | 0.00 | 0.89 | -21.34 | 154.44 | 25.59 | 223.33 | 0.5885 | 873.0 | 724.5 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -18.60 | 153.62 | 24.77 | 226.00 | 0.5540 | 579.0 | 483.5 | |
| 0.00 | 2.00 | 0.00 | 1.12 | -9.82 | 152.55 | 23.70 | 238.93 | 0.4643 | 672.0 | 491.8 | |
| 0.00 | 2.00 | 0.00 | 1.17 | -17.69 | 152.92 | 24.07 | 226.48 | 0.5379 | 738.0 | 631.7 | |
| 0.00 | 1.91 | 0.00 | 1.11 | -17.09 | 152.63 | 23.77 | 227.00 | 0.5290 | 644.0 | 555.2 | |
| 0.00 | 0.64 | 0.00 | 0.37 | -17.53 | 152.23 | 23.38 | 225.89 | 0.5291 | 789.0 | 656.6 | |
| 0.00 | 2.00 | 0.00 | 1.17 | -17.80 | 152.16 | 23.31 | 225.44 | 0.5309 | 711.0 | 585.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -19.40 | 151.76 | 22.91 | 222.76 | 0.5430 | 619.0 | 511.6 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -17.59 | 150.75 | 21.90 | 223.98 | 0.5140 | 774.0 | 618.8 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -21.07 | 150.54 | 21.69 | 219.10 | 0.5488 | 552.0 | 568.2 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -21.27 | 150.54 | 21.68 | 218.85 | 0.5510 | 618.0 | 532.3 | |
| 0.00 | 3.72 | 0.00 | 2.13 | -17.59 | 149.68 | 20.83 | 222.58 | 0.5030 | 725.0 | 707.7 | |
| 0.00 | 2.54 | 0.00 | 1.45 | -17.74 | 149.33 | 20.47 | 221.88 | 0.5010 | 709.0 | 580.8 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -17.41 | 149.22 | 20.37 | 222.20 | 0.4963 | 764.0 | 572.2 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -22.06 | 149.74 | 20.89 | 216.89 | 0.5526 | 251.0 | 362.4 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -14.70 | 148.73 | 19.88 | 225.61 | 0.4622 | 733.0 | 567.4 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -20.59 | 147.93 | 19.08 | 216.22 | 0.5199 | 772.0 | 597.5 | |
| 0.00 | 2.18 | 0.00 | 1.26 | -20.92 | 147.80 | 18.95 | 215.64 | 0.5227 | 840.0 | 597.4 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -21.26 | 147.85 | 18.99 | 215.30 | 0.5270 | 552.0 | 480.1 | |
| 0.00 | 0.64 | 0.00 | 0.37 | -20.99 | 147.64 | 18.79 | 215.33 | 0.5220 | 693.0 | 628.1 | |
| 0.45 | 1.63 | 0.26 | 0.94 | -20.60 | 147.14 | 18.29 | 215.08 | 0.5132 | 867.2 | 688.4 | |
| 0.00 | 1.91 | 0.00 | 1.09 | -19.85 | 146.50 | 17.65 | 215.05 | 0.4986 | 626.0 | 457.9 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -20.62 | 146.53 | 17.67 | 214.16 | 0.5081 | 787.0 | 599.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -20.44 | 145.86 | 17.01 | 213.37 | 0.5003 | -423.0 | -401.7 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -11.76 | 145.11 | 16.26 | 224.96 | 0.3897 | 845.0 | 668.6 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -20.94 | 145.74 | 16.89 | 212.61 | 0.5055 | -410.0 | -310.5 | |
| 0.00 | 2.91 | 0.00 | 1.62 | -17.76 | 145.04 | 16.19 | 215.41 | 0.4602 | -911.0 | -770.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -18.15 | 145.01 | 16.16 | 214.85 | 0.4648 | -799.0 | -689.3 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -18.70 | 144.23 | 15.38 | 212.85 | 0.4649 | -703.0 | -683.6 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -23.99 | 144.77 | 15.92 | 207.96 | 0.5365 | -731.0 | -585.2 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -22.19 | 144.49 | 15.64 | 209.32 | 0.5116 | -676.0 | -546.9 | |
| 0.00 | 0.64 | 0.00 | 0.37 | -24.27 | 143.59 | 14.74 | 205.94 | 0.5323 | -697.0 | -585.1 | |
| 0.00 | 0.64 | 0.00 | 0.37 | -24.16 | 143.34 | 14.49 | 205.66 | 0.5292 | -609.0 | -516.6 | |
| 0.00 | 1.82 | 0.00 | 1.06 | -24.06 | 143.19 | 14.34 | 205.52 | 0.5268 | -446.0 | -486.8 | |
| 0.00 | 1.73 | 0.00 | 0.99 | -23.48 | 141.96 | 13.11 | 204.10 | 0.5114 | -755.0 | -512.8 | |
| 0.00 | 1.91 | 0.00 | 1.13 | -26.63 | 141.99 | 13.14 | 201.61 | 0.5539 | -572.0 | -531.4 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -27.44 | 141.77 | 12.92 | 200.70 | 0.5636 | -670.0 | -560.5 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -27.51 | 141.57 | 12.72 | 200.35 | 0.5634 | -630.0 | -498.5 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -23.30 | 139.64 | 10.78 | 200.37 | 0.4957 | -769.0 | -643.7 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -27.85 | 128.61 | -0.24 | 179.59 | 0.5350 | -631.0 | -472.9 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -25.10 | 121.93 | -6.92 | 167.48 | 0.5052 | -780.0 | -620.1 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -24.40 | 119.37 | -9.48 | 162.64 | 0.5049 | -647.0 | -579.3 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -25.48 | 113.05 | -15.80 | 153.58 | 0.5547 | -527.0 | -435.2 | |
| 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. | |