SDO HMI 2014-08-09 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.23 | 107.31 | 2.62 | 54.25 | 9.14 | 174.37 | 10.17 | 281.41 | 0.1890 | 137.9 | 117.2 | |
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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 | 1.26 | 0.00 | 0.66 | 6.42 | 182.61 | 18.41 | 271.36 | 0.3153 | -713.0 | -569.9 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 6.73 | 182.33 | 18.13 | 272.37 | 0.3107 | -926.0 | -798.5 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 6.90 | 182.08 | 17.88 | 272.90 | 0.3066 | -690.0 | -583.7 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 10.82 | 182.06 | 17.86 | 285.56 | 0.3141 | -503.0 | -476.0 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 7.15 | 181.71 | 17.51 | 273.77 | 0.3005 | -642.0 | -510.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 10.84 | 181.73 | 17.54 | 285.82 | 0.3089 | -704.0 | -657.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 11.24 | 181.60 | 17.40 | 287.20 | 0.3084 | -656.0 | -555.6 | |
| 0.00 | 2.98 | 0.00 | 1.53 | 9.62 | 179.70 | 15.50 | 283.16 | 0.2718 | -874.0 | -794.3 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 9.32 | 179.66 | 15.46 | 282.09 | 0.2702 | -1036.0 | -897.6 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 8.17 | 179.45 | 15.25 | 277.91 | 0.2640 | -887.0 | -770.0 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 8.53 | 179.37 | 15.17 | 279.34 | 0.2634 | -348.0 | -447.7 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 6.42 | 179.00 | 14.80 | 271.22 | 0.2551 | -756.0 | -556.7 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 8.56 | 178.48 | 14.28 | 279.90 | 0.2487 | -908.0 | -733.2 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 8.35 | 178.18 | 13.98 | 279.23 | 0.2433 | -682.0 | -428.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 10.40 | 177.83 | 13.63 | 287.80 | 0.2445 | -958.0 | -766.9 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 11.72 | 177.83 | 13.63 | 292.85 | 0.2514 | -824.0 | -680.2 | |
| 0.00 | 2.89 | 0.00 | 1.47 | 8.42 | 176.96 | 12.76 | 280.23 | 0.2229 | -937.0 | -758.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 8.73 | 176.81 | 12.61 | 281.71 | 0.2213 | -778.0 | -627.0 | |
| 0.00 | 2.89 | 0.00 | 1.47 | 8.70 | 176.59 | 12.39 | 281.77 | 0.2176 | -865.0 | -816.5 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 8.89 | 176.47 | 12.27 | 282.72 | 0.2162 | -727.0 | -674.1 | |
| 0.00 | 7.04 | 0.00 | 3.57 | 8.62 | 176.21 | 12.01 | 281.70 | 0.2110 | -1001.0 | -839.8 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 9.99 | 176.10 | 11.90 | 288.12 | 0.2146 | -810.0 | -579.3 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 9.23 | 176.01 | 11.81 | 284.76 | 0.2098 | -826.0 | -692.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 8.96 | 176.00 | 11.80 | 283.49 | 0.2087 | -820.0 | -657.3 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.00 | 175.37 | 11.17 | 284.36 | 0.1984 | -739.0 | -598.4 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 11.63 | 175.25 | 11.05 | 296.74 | 0.2112 | 632.0 | 441.7 | |
| 0.00 | 1.99 | 0.00 | 1.00 | 9.37 | 175.07 | 10.87 | 286.57 | 0.1950 | -846.0 | -718.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 9.69 | 174.42 | 10.22 | 289.13 | 0.1860 | 701.0 | 523.5 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 9.79 | 174.24 | 10.04 | 289.93 | 0.1835 | 1091.0 | 831.7 | |
| 0.00 | 3.07 | 0.00 | 1.55 | 9.95 | 173.84 | 9.64 | 291.49 | 0.1780 | 737.0 | 615.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 9.71 | 173.77 | 9.57 | 290.33 | 0.1755 | 842.0 | 755.7 | |
| 0.90 | 4.15 | 0.45 | 2.09 | 8.46 | 173.51 | 9.31 | 283.67 | 0.1655 | 1003.5 | 818.4 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 10.71 | 173.58 | 9.38 | 296.03 | 0.1790 | 872.0 | 709.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 8.89 | 173.43 | 9.23 | 286.31 | 0.1659 | 795.0 | 651.1 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 10.29 | 173.31 | 9.12 | 294.42 | 0.1720 | 886.0 | 735.6 | |
| 0.00 | 2.62 | 0.00 | 1.31 | 8.38 | 173.20 | 9.00 | 283.57 | 0.1599 | 748.0 | 671.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 9.14 | 173.19 | 8.99 | 288.17 | 0.1631 | 894.0 | 740.1 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 9.05 | 173.06 | 8.86 | 287.86 | 0.1606 | 929.0 | 776.8 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 8.66 | 172.71 | 8.51 | 286.07 | 0.1529 | 1089.0 | 892.8 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 8.14 | 172.70 | 8.50 | 282.76 | 0.1507 | 789.0 | 649.1 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 10.30 | 172.66 | 8.46 | 296.06 | 0.1619 | 888.0 | 752.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.36 | 172.61 | 8.41 | 284.29 | 0.1500 | 825.0 | 659.9 | |
| 0.00 | 1.99 | 0.00 | 0.99 | 8.15 | 172.39 | 8.19 | 283.23 | 0.1455 | 831.0 | 645.7 | |
| 0.00 | 2.44 | 0.00 | 1.22 | 10.31 | 172.41 | 8.21 | 296.74 | 0.1580 | 892.0 | 745.0 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 8.58 | 172.30 | 8.10 | 286.22 | 0.1458 | 856.0 | 660.3 | |
| 0.00 | 3.70 | 0.00 | 1.85 | 8.85 | 172.22 | 8.02 | 288.21 | 0.1457 | 894.0 | 851.4 | |
| 1.08 | 4.06 | 0.54 | 2.04 | 10.01 | 172.18 | 7.98 | 295.59 | 0.1523 | 1100.6 | 873.3 | |
| 0.99 | 6.32 | 0.50 | 3.17 | 9.65 | 171.89 | 7.69 | 294.13 | 0.1453 | 1171.8 | 910.7 | |
| 2.26 | 3.79 | 1.13 | 1.90 | 9.44 | 171.55 | 7.35 | 293.72 | 0.1384 | 1125.5 | 838.2 | |
| 0.00 | 1.99 | 0.00 | 0.99 | 9.44 | 171.21 | 7.01 | 294.74 | 0.1331 | 999.0 | 888.6 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 9.87 | 171.18 | 6.98 | 297.68 | 0.1359 | 1080.0 | 913.8 | |
| 0.00 | 2.80 | 0.00 | 1.40 | 9.08 | 171.07 | 6.87 | 292.55 | 0.1286 | 897.0 | 757.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 8.05 | 170.59 | 6.39 | 285.74 | 0.1150 | 717.0 | 435.0 | |
| 0.00 | 2.17 | 0.00 | 1.08 | 8.84 | 168.04 | 3.84 | 303.82 | 0.0801 | 865.0 | 648.3 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 9.12 | 168.01 | 3.82 | 306.79 | 0.0824 | 927.0 | 729.2 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 5.35 | 158.97 | -5.23 | 100.25 | 0.0927 | 942.0 | 781.8 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 12.36 | 157.84 | -6.36 | 45.55 | 0.1522 | 706.0 | 546.3 | |
| 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. | |