SDO HMI 2014-07-04 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.59 | 186.48 | 21.03 | 94.35 | 11.53 | 278.85 | 7.74 | 318.14 | 0.2016 | -312.1 | -246.2 | |
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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 | 1.63 | 0.00 | 0.89 | 14.86 | 293.75 | 22.64 | 298.92 | 0.4268 | -921.0 | -666.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 9.13 | 288.51 | 17.40 | 289.59 | 0.3148 | -667.0 | -520.7 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 9.10 | 288.32 | 17.21 | 289.69 | 0.3116 | -803.0 | -533.1 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 11.56 | 281.73 | 10.62 | 308.90 | 0.2329 | -904.0 | -705.3 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 13.08 | 281.66 | 10.55 | 313.90 | 0.2487 | -1011.0 | -876.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 11.13 | 281.58 | 10.47 | 307.77 | 0.2266 | -892.0 | -750.6 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 10.95 | 281.39 | 10.28 | 307.62 | 0.2221 | -893.0 | -791.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.51 | 280.84 | 9.73 | 303.44 | 0.2006 | -921.0 | -774.6 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 13.86 | 281.00 | 9.89 | 317.98 | 0.2501 | -750.0 | -592.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 10.38 | 280.52 | 9.41 | 307.84 | 0.2045 | -833.0 | -701.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 10.44 | 280.30 | 9.19 | 308.73 | 0.2022 | -831.0 | -678.7 | |
| 0.91 | 98.97 | 0.46 | 50.06 | 10.96 | 280.29 | 9.17 | 310.78 | 0.2077 | -843.4 | -662.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 13.96 | 280.40 | 9.29 | 319.99 | 0.2447 | -912.0 | -716.9 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 9.03 | 280.17 | 9.06 | 303.15 | 0.1865 | -877.0 | -718.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 11.67 | 280.25 | 9.14 | 313.44 | 0.2151 | -567.0 | -358.6 | |
| 0.54 | 2.54 | 0.27 | 1.28 | 9.28 | 280.08 | 8.97 | 304.51 | 0.1875 | -1206.8 | -1035.2 | |
| 4.54 | -12.00 | 2.30 | -12.00 | 11.03 | 280.10 | 8.99 | 311.59 | 0.2059 | -1042.0 | 999999 | |
| 9.35 | -12.00 | 4.73 | -12.00 | 11.18 | 279.82 | 8.71 | 313.04 | 0.2042 | -1210.0 | 999999 | |
| 6.36 | -12.00 | 3.22 | -12.00 | 11.46 | 279.80 | 8.69 | 314.11 | 0.2071 | -1044.3 | 999999 | |
| 2.36 | -12.00 | 1.19 | -12.00 | 10.57 | 279.77 | 8.66 | 310.88 | 0.1966 | -1122.6 | 999999 | |
| 13.44 | -12.00 | 6.79 | -12.00 | 10.94 | 279.75 | 8.64 | 312.36 | 0.2005 | -1342.5 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 10.42 | 279.36 | 8.25 | 311.64 | 0.1897 | -503.0 | -347.7 | |
| 0.00 | 1.82 | 0.00 | 0.91 | 7.78 | 279.26 | 8.15 | 299.57 | 0.1623 | -775.0 | -565.3 | |
| 2.27 | -12.00 | 1.15 | -12.00 | 11.13 | 279.22 | 8.11 | 314.84 | 0.1962 | -1164.0 | 999999 | |
| 0.82 | 6.81 | 0.41 | 3.42 | 8.21 | 279.12 | 8.01 | 302.31 | 0.1639 | -1252.3 | -918.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 7.55 | 278.70 | 7.59 | 299.97 | 0.1518 | 935.0 | 728.9 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 12.80 | 278.74 | 7.63 | 322.12 | 0.2118 | -810.0 | -585.3 | |
| 0.00 | 3.72 | 0.00 | 1.88 | 11.87 | 278.12 | 7.00 | 321.58 | 0.1929 | -893.0 | -808.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 18.20 | 277.92 | 6.81 | 336.46 | 0.2831 | 820.0 | 631.4 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 11.76 | 277.64 | 6.53 | 323.11 | 0.1863 | -911.0 | -812.0 | |
| 1.00 | 2.45 | 0.51 | 1.24 | 13.55 | 277.38 | 6.26 | 329.38 | 0.2092 | 951.4 | 726.1 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.01 | 277.24 | 6.13 | 301.91 | 0.1254 | 907.0 | 717.3 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 12.31 | 277.09 | 5.98 | 327.20 | 0.1888 | -783.0 | -608.6 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 11.36 | 276.51 | 5.40 | 326.90 | 0.1696 | 904.0 | 775.5 | |
| 0.00 | 2.63 | 0.00 | 1.33 | 13.83 | 276.41 | 5.30 | 334.04 | 0.2056 | -807.0 | -665.9 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 13.00 | 275.85 | 4.74 | 334.60 | 0.1887 | 897.0 | 647.2 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.31 | 275.77 | 4.65 | 335.71 | 0.1928 | 761.0 | 633.7 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 13.19 | 275.57 | 4.46 | 336.33 | 0.1896 | 1314.0 | 1045.8 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 12.79 | 275.54 | 4.42 | 335.61 | 0.1830 | 835.0 | 681.7 | |
| 0.00 | 2.18 | 0.00 | 1.10 | 12.54 | 275.50 | 4.39 | 335.21 | 0.1789 | 980.0 | 810.3 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 12.29 | 275.46 | 4.35 | 334.78 | 0.1748 | 817.0 | 662.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 12.54 | 275.25 | 4.14 | 336.46 | 0.1772 | 948.0 | 763.8 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 12.85 | 275.22 | 4.11 | 337.29 | 0.1819 | 977.0 | 869.9 | |
| 0.00 | 2.54 | 0.00 | 1.28 | 11.71 | 275.17 | 4.06 | 334.79 | 0.1636 | 1001.0 | 717.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 13.22 | 275.10 | 3.99 | 338.65 | 0.1870 | 975.0 | 753.8 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 13.90 | 275.02 | 3.91 | 340.32 | 0.1975 | 802.0 | 669.1 | |
| 0.00 | 2.36 | 0.00 | 1.19 | 12.76 | 275.00 | 3.89 | 338.19 | 0.1790 | 919.0 | 716.7 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 12.54 | 274.97 | 3.86 | 337.90 | 0.1753 | 909.0 | 699.3 | |
| 0.00 | 4.18 | 0.00 | 2.11 | 13.25 | 274.82 | 3.71 | 340.09 | 0.1858 | 796.0 | 729.5 | |
| 0.00 | 2.72 | 0.00 | 1.38 | 13.87 | 274.77 | 3.66 | 341.44 | 0.1956 | 811.0 | 767.9 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 13.94 | 274.14 | 3.03 | 344.55 | 0.1935 | 943.0 | 742.6 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 14.16 | 273.80 | 2.69 | 346.50 | 0.1956 | 1065.0 | 843.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.34 | 273.64 | 2.53 | 347.46 | 0.1982 | 919.0 | 768.0 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 15.31 | 273.53 | 2.42 | 348.98 | 0.2140 | 759.0 | 614.6 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 14.53 | 273.33 | 2.22 | 349.15 | 0.2002 | 921.0 | 707.3 | |
| 0.00 | 2.54 | 0.00 | 1.29 | 15.00 | 272.96 | 1.85 | 351.31 | 0.2071 | 812.0 | 721.4 | |
| 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. | |