SDO HMI 2014-07-04 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.51 | 221.68 | 20.91 | 111.72 | 11.58 | 278.67 | 5.89 | 325.42 | 0.1833 | -262.4 | -235.7 | |
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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 | 0.54 | 0.00 | 0.30 | 14.94 | 294.23 | 21.46 | 300.31 | 0.4111 | -815.0 | -611.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 12.55 | 291.05 | 18.27 | 298.28 | 0.3490 | -611.0 | -490.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 11.88 | 284.23 | 11.45 | 307.94 | 0.2475 | -829.0 | -682.9 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 11.20 | 281.52 | 8.74 | 313.06 | 0.2049 | -892.0 | -753.3 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 13.12 | 281.55 | 8.77 | 319.22 | 0.2285 | -1013.0 | -844.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.99 | 281.41 | 8.64 | 312.60 | 0.2012 | -1090.0 | -833.1 | |
| 0.00 | 2.63 | 0.00 | 1.33 | 10.77 | 281.31 | 8.54 | 312.11 | 0.1975 | -975.0 | -841.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.86 | 280.98 | 8.20 | 323.19 | 0.2322 | -829.0 | -595.8 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 10.48 | 280.46 | 7.68 | 313.90 | 0.1833 | -921.0 | -569.1 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 13.99 | 280.31 | 7.54 | 325.78 | 0.2274 | -794.0 | -695.0 | |
| 3.09 | 126.51 | 1.56 | 63.74 | 11.00 | 280.16 | 7.39 | 317.06 | 0.1861 | -933.6 | -620.3 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 9.07 | 280.05 | 7.28 | 309.22 | 0.1622 | -896.0 | -679.5 | |
| 3.81 | -11.00 | 1.92 | -11.00 | 11.12 | 280.04 | 7.26 | 317.99 | 0.1862 | -1108.6 | 999999 | |
| 0.82 | 4.00 | 0.41 | 2.01 | 9.34 | 280.00 | 7.22 | 310.76 | 0.1645 | -1254.9 | -881.6 | |
| 3.91 | -11.00 | 1.97 | -11.00 | 10.57 | 279.84 | 7.06 | 316.68 | 0.1770 | -1075.3 | 999999 | |
| 8.81 | -11.00 | 4.44 | -11.00 | 11.22 | 279.82 | 7.05 | 319.18 | 0.1849 | -1207.7 | 999999 | |
| 9.99 | -11.00 | 5.03 | -11.00 | 10.94 | 279.78 | 7.01 | 318.32 | 0.1810 | -1380.4 | 999999 | |
| 4.54 | -11.00 | 2.29 | -11.00 | 11.50 | 279.80 | 7.02 | 320.26 | 0.1883 | -1032.2 | 999999 | |
| 2.09 | -11.00 | 1.05 | -11.00 | 11.71 | 279.62 | 6.84 | 321.73 | 0.1892 | -827.3 | 999999 | |
| 1.09 | -11.00 | 0.55 | -11.00 | 11.34 | 279.58 | 6.80 | 320.63 | 0.1838 | -1102.7 | 999999 | |
| 1.36 | -11.00 | 0.69 | -11.00 | 11.16 | 279.51 | 6.73 | 320.24 | 0.1807 | -1188.1 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 8.61 | 279.33 | 6.55 | 309.84 | 0.1476 | -851.0 | -728.9 | |
| 0.91 | 8.72 | 0.45 | 4.36 | 8.16 | 278.95 | 6.17 | 308.99 | 0.1376 | -1054.2 | -987.1 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 13.66 | 278.95 | 6.17 | 330.06 | 0.2102 | -641.0 | -494.4 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 7.61 | 278.54 | 5.76 | 307.59 | 0.1262 | 870.0 | 733.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.10 | 278.29 | 5.52 | 333.71 | 0.2116 | -851.0 | -695.7 | |
| 0.00 | 2.45 | 0.00 | 1.23 | 11.94 | 278.18 | 5.41 | 328.70 | 0.1782 | -923.0 | -806.0 | |
| 0.00 | 4.18 | 0.00 | 2.11 | 13.49 | 277.46 | 4.69 | 335.97 | 0.1960 | 580.0 | 488.0 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 6.89 | 277.20 | 4.43 | 309.81 | 0.1002 | 925.0 | 738.4 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 7.07 | 277.17 | 4.40 | 311.38 | 0.1019 | 885.0 | 663.5 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 12.31 | 277.09 | 4.32 | 335.03 | 0.1751 | -661.0 | -503.3 | |
| 0.00 | 2.27 | 0.00 | 1.14 | 11.39 | 276.52 | 3.74 | 335.75 | 0.1565 | 792.0 | 676.8 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 13.71 | 276.46 | 3.68 | 341.06 | 0.1932 | -849.0 | -684.2 | |
| 0.00 | 5.72 | 0.00 | 2.88 | 12.97 | 275.98 | 3.20 | 342.16 | 0.1785 | 889.0 | 715.5 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 11.86 | 275.74 | 2.97 | 341.33 | 0.1591 | 719.0 | 508.1 | |
| 1.09 | 2.45 | 0.55 | 1.23 | 13.16 | 275.60 | 2.83 | 344.42 | 0.1798 | 1191.3 | 990.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 12.54 | 275.57 | 2.79 | 343.63 | 0.1693 | 776.0 | 510.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.56 | 275.33 | 2.55 | 346.43 | 0.1853 | 905.0 | 747.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 12.94 | 275.26 | 2.48 | 345.95 | 0.1747 | 1065.0 | 926.8 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 11.71 | 275.12 | 2.34 | 344.80 | 0.1534 | 1151.0 | 904.4 | |
| 0.00 | 3.09 | 0.00 | 1.55 | 13.16 | 275.04 | 2.27 | 347.41 | 0.1774 | 450.0 | 588.0 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 13.81 | 274.98 | 2.21 | 348.47 | 0.1882 | 825.0 | 736.5 | |
| 0.00 | 3.81 | 0.00 | 1.92 | 12.60 | 274.94 | 2.17 | 347.24 | 0.1677 | 940.0 | 798.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 11.49 | 274.90 | 2.12 | 345.81 | 0.1489 | 836.0 | 524.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 13.38 | 274.73 | 1.95 | 349.33 | 0.1800 | 1048.0 | 873.3 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 13.87 | 274.67 | 1.90 | 350.13 | 0.1883 | 1007.0 | 775.2 | |
| 0.00 | 2.09 | 0.00 | 1.05 | 13.31 | 274.57 | 1.80 | 350.11 | 0.1785 | 1032.0 | 772.3 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 14.90 | 274.21 | 1.43 | 353.18 | 0.2046 | 816.0 | 606.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.33 | 273.83 | 1.06 | 355.15 | 0.2114 | -591.0 | -374.6 | |
| 0.00 | 2.82 | 0.00 | 1.42 | 14.25 | 273.76 | 0.99 | 355.00 | 0.1926 | 998.0 | 848.1 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 14.09 | 273.64 | 0.86 | 355.57 | 0.1898 | 894.0 | 772.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 14.56 | 273.61 | 0.83 | 355.90 | 0.1977 | 802.0 | 600.1 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 14.37 | 273.58 | 0.80 | 355.99 | 0.1945 | 1065.0 | 871.9 | |
| 0.00 | 4.36 | 0.00 | 2.20 | 14.43 | 273.26 | 0.49 | 357.58 | 0.1953 | 947.0 | 827.3 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 14.59 | 273.07 | 0.30 | 358.54 | 0.1979 | 677.0 | 557.4 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 14.93 | 272.88 | 0.11 | 359.48 | 0.2037 | 890.0 | 692.5 | |
| 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. | |