SDO HMI 2014-07-04 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.33 | 221.61 | 22.80 | 111.61 | 11.70 | 278.73 | 5.40 | 327.89 | 0.1802 | -303.0 | -268.0 | |
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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 | 0.91 | 0.00 | 0.49 | 15.21 | 293.63 | 20.30 | 302.20 | 0.3974 | -760.0 | -600.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 11.98 | 284.37 | 11.04 | 309.24 | 0.2430 | -790.0 | -608.6 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 13.11 | 281.91 | 8.59 | 319.83 | 0.2264 | -777.0 | -657.4 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 11.27 | 281.51 | 8.18 | 315.17 | 0.1988 | -843.0 | -703.3 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 13.12 | 281.50 | 8.18 | 321.20 | 0.2220 | -827.0 | -811.7 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 11.02 | 281.41 | 8.08 | 314.62 | 0.1946 | -987.0 | -836.4 | |
| 0.00 | 5.00 | 0.00 | 2.52 | 10.81 | 281.31 | 7.98 | 314.16 | 0.1909 | -801.0 | -776.1 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 13.87 | 280.93 | 7.60 | 325.24 | 0.2262 | -834.0 | -681.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 10.51 | 280.48 | 7.16 | 316.06 | 0.1773 | -761.0 | -572.8 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 14.00 | 280.30 | 6.97 | 327.82 | 0.2221 | -868.0 | -694.8 | |
| 0.00 | 0.73 | 0.00 | 0.36 | 9.07 | 280.08 | 6.75 | 311.34 | 0.1553 | -764.0 | -629.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.25 | 280.08 | 6.75 | 312.21 | 0.1574 | -905.0 | -775.2 | |
| 1.09 | 2.91 | 0.55 | 1.46 | 9.38 | 279.93 | 6.60 | 313.45 | 0.1569 | -1206.4 | -913.8 | |
| 16.98 | 128.25 | 8.55 | 64.55 | 11.03 | 279.90 | 6.57 | 320.46 | 0.1773 | -1255.1 | -598.2 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.98 | 279.86 | 6.53 | 311.82 | 0.1514 | -812.0 | -649.9 | |
| 4.72 | -14.00 | 2.37 | -14.00 | 10.57 | 279.83 | 6.50 | 319.03 | 0.1705 | -951.3 | 999999 | |
| 8.45 | -14.00 | 4.25 | -14.00 | 11.22 | 279.78 | 6.45 | 321.64 | 0.1785 | -1209.6 | 999999 | |
| 5.18 | -14.00 | 2.61 | -14.00 | 11.53 | 279.76 | 6.43 | 322.82 | 0.1824 | -1048.4 | 999999 | |
| 1.91 | -14.00 | 0.96 | -14.00 | 11.74 | 279.61 | 6.28 | 324.18 | 0.1838 | -815.4 | 999999 | |
| 0.91 | -14.00 | 0.46 | -14.00 | 11.38 | 279.57 | 6.24 | 323.12 | 0.1783 | -1103.8 | 999999 | |
| 1.45 | -14.00 | 0.73 | -14.00 | 11.19 | 279.16 | 5.83 | 324.33 | 0.1716 | -1152.4 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 11.81 | 279.11 | 5.78 | 326.59 | 0.1798 | -695.0 | -677.0 | |
| 4.00 | 7.45 | 2.00 | 3.72 | 8.31 | 278.95 | 5.62 | 312.51 | 0.1320 | -1153.6 | -920.6 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 8.77 | 278.55 | 5.22 | 317.09 | 0.1328 | -852.0 | -722.0 | |
| 0.00 | 5.18 | 0.00 | 2.60 | 11.97 | 278.20 | 4.88 | 331.34 | 0.1742 | -850.0 | -727.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.10 | 278.25 | 4.92 | 336.22 | 0.2073 | -815.0 | -555.0 | |
| 0.00 | 3.54 | 0.00 | 1.78 | 11.08 | 278.03 | 4.70 | 329.52 | 0.1594 | -807.0 | -657.6 | |
| 0.00 | 2.63 | 0.00 | 1.35 | 18.14 | 277.87 | 4.55 | 343.69 | 0.2694 | 665.0 | 588.3 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 13.12 | 276.57 | 3.24 | 342.25 | 0.1812 | -630.0 | -562.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.42 | 276.45 | 3.12 | 339.48 | 0.1529 | 863.0 | 694.4 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 13.71 | 276.48 | 3.15 | 343.64 | 0.1905 | -853.0 | -708.8 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 13.68 | 276.17 | 2.84 | 345.15 | 0.1885 | -737.0 | -552.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 12.88 | 276.09 | 2.76 | 344.33 | 0.1748 | 800.0 | 634.2 | |
| 0.00 | 3.00 | 0.00 | 1.51 | 13.03 | 275.94 | 2.61 | 345.40 | 0.1767 | 836.0 | 797.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 13.28 | 275.78 | 2.46 | 346.56 | 0.1802 | 862.0 | 722.5 | |
| 0.64 | 2.54 | 0.32 | 1.28 | 13.16 | 275.66 | 2.33 | 347.07 | 0.1777 | 1208.6 | 1039.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 12.72 | 275.59 | 2.26 | 346.86 | 0.1701 | 905.0 | 749.0 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 13.59 | 275.32 | 1.99 | 349.38 | 0.1838 | 905.0 | 811.0 | |
| 0.00 | 3.18 | 0.00 | 1.60 | 12.91 | 275.28 | 1.95 | 348.83 | 0.1722 | 1020.0 | 872.7 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 11.71 | 275.11 | 1.78 | 348.31 | 0.1512 | 1156.0 | 994.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 13.75 | 274.97 | 1.65 | 351.31 | 0.1855 | 885.0 | 765.2 | |
| 0.00 | 3.27 | 0.00 | 1.64 | 12.63 | 274.93 | 1.60 | 350.50 | 0.1664 | 886.0 | 795.9 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 11.49 | 274.89 | 1.57 | 349.44 | 0.1468 | 716.0 | 530.2 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 13.87 | 274.75 | 1.43 | 352.54 | 0.1871 | 838.0 | 709.5 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 13.37 | 274.69 | 1.36 | 352.53 | 0.1784 | 1133.0 | 905.2 | |
| 0.00 | 2.27 | 0.00 | 1.14 | 13.28 | 274.53 | 1.20 | 353.32 | 0.1765 | 995.0 | 804.6 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 14.90 | 274.20 | 0.87 | 355.87 | 0.2036 | 909.0 | 701.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.59 | 273.97 | 0.64 | 356.54 | 0.1810 | 900.0 | 773.6 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 14.46 | 273.85 | 0.52 | 357.43 | 0.1958 | 785.0 | 688.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.40 | 273.85 | 0.52 | 357.61 | 0.2118 | -637.0 | -440.2 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 14.24 | 273.75 | 0.42 | 357.85 | 0.1920 | 991.0 | 883.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.59 | 273.60 | 0.27 | 358.69 | 0.1978 | 821.0 | 640.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.40 | 273.53 | 0.20 | 358.98 | 0.1946 | 1056.0 | 843.5 | |
| 0.00 | 3.45 | 0.00 | 1.74 | 14.37 | 273.22 | -0.11 | 0.56 | 0.1941 | 1001.0 | 860.1 | |
| 0.00 | 2.54 | 0.00 | 1.29 | 14.62 | 273.09 | -0.24 | 1.16 | 0.1984 | 879.0 | 623.1 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 14.87 | 272.87 | -0.46 | 2.19 | 0.2028 | 818.0 | 687.0 | |
| 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. | |