SDO HMI 2014-04-21 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.60 | 239.91 | 29.08 | 120.87 | -11.11 | 184.96 | 8.33 | 232.95 | 0.1824 | 452.8 | 302.3 | |
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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 | 2.40 | 0.00 | 1.23 | -14.03 | 188.44 | 11.81 | 231.68 | 0.2542 | 884.0 | 777.9 | |
| 0.00 | 1.51 | 0.00 | 0.77 | -13.75 | 188.43 | 11.80 | 232.53 | 0.2513 | 704.0 | 530.2 | |
| 0.89 | 3.64 | 0.45 | 1.85 | -11.12 | 187.93 | 11.30 | 241.04 | 0.2208 | 937.9 | 783.6 | |
| 0.00 | 1.69 | 0.00 | 0.86 | -11.36 | 187.76 | 11.13 | 239.68 | 0.2202 | 824.0 | 684.6 | |
| 20.77 | 40.74 | 10.53 | 20.65 | -10.52 | 187.69 | 11.06 | 243.05 | 0.2126 | 1154.1 | 767.4 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -9.34 | 187.25 | 10.62 | 247.47 | 0.1978 | 721.0 | 548.0 | |
| 0.00 | 1.69 | 0.00 | 0.85 | -9.55 | 187.26 | 10.63 | 246.49 | 0.1992 | 908.0 | 759.4 | |
| 0.00 | 2.40 | 0.00 | 1.21 | -11.34 | 187.29 | 10.66 | 238.73 | 0.2131 | 789.0 | 692.2 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -11.10 | 187.18 | 10.55 | 239.49 | 0.2095 | 946.0 | 680.1 | |
| 0.00 | 1.78 | 0.00 | 0.90 | -13.19 | 187.23 | 10.60 | 231.56 | 0.2298 | 855.0 | 658.7 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -9.65 | 187.04 | 10.41 | 245.64 | 0.1965 | 763.0 | 600.6 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -11.37 | 187.01 | 10.38 | 237.93 | 0.2093 | 741.0 | 491.4 | |
| 3.02 | 17.84 | 1.52 | 9.00 | -9.56 | 186.88 | 10.25 | 245.75 | 0.1934 | 1145.9 | 805.7 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -11.07 | 186.93 | 10.30 | 239.02 | 0.2056 | 641.0 | 413.1 | |
| 4.97 | -13.00 | 2.51 | -13.00 | -9.29 | 186.78 | 10.15 | 246.86 | 0.1901 | 1161.4 | 999999 | |
| 0.00 | 1.60 | 0.00 | 0.81 | -10.71 | 186.73 | 10.10 | 240.11 | 0.1997 | -678.0 | -519.4 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -8.39 | 186.61 | 9.97 | 251.13 | 0.1819 | 778.0 | 488.3 | |
| 0.00 | 2.31 | 0.00 | 1.16 | -8.84 | 186.59 | 9.96 | 248.74 | 0.1841 | 883.0 | 713.3 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -9.60 | 186.54 | 9.91 | 244.88 | 0.1884 | 1013.0 | 840.1 | |
| 2.84 | 4.53 | 1.44 | 2.29 | -11.38 | 186.54 | 9.91 | 236.74 | 0.2026 | 1107.1 | 763.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -12.78 | 186.59 | 9.96 | 231.36 | 0.2169 | 951.0 | 740.4 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -8.99 | 186.28 | 9.65 | 247.35 | 0.1802 | 962.0 | 824.7 | |
| 0.00 | 0.71 | 0.00 | 0.36 | -8.39 | 186.20 | 9.57 | 250.40 | 0.1754 | 431.0 | 582.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -10.81 | 186.27 | 9.64 | 238.54 | 0.1937 | -385.0 | -291.9 | |
| 3.46 | 14.74 | 1.75 | 7.44 | -11.48 | 186.10 | 9.47 | 235.18 | 0.1974 | 1103.3 | 838.0 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -10.48 | 185.83 | 9.19 | 238.88 | 0.1844 | -567.0 | -442.9 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -13.03 | 185.69 | 9.06 | 227.82 | 0.2079 | -667.0 | -543.2 | |
| 0.00 | 4.17 | 0.00 | 2.10 | -11.51 | 185.58 | 8.95 | 233.51 | 0.1904 | 1027.0 | 867.8 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -12.25 | 185.35 | 8.72 | 229.77 | 0.1949 | 815.0 | 472.1 | |
| 0.00 | 2.31 | 0.00 | 1.16 | -11.15 | 185.29 | 8.66 | 234.22 | 0.1828 | 1043.0 | 696.4 | |
| 1.24 | 15.00 | 0.63 | 7.55 | -10.61 | 185.18 | 8.55 | 236.43 | 0.1761 | -888.4 | -573.1 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -8.08 | 184.78 | 8.15 | 249.40 | 0.1506 | 830.0 | 701.8 | |
| 0.00 | 1.78 | 0.00 | 0.89 | -7.94 | 183.92 | 7.29 | 248.25 | 0.1359 | -805.0 | -606.8 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -10.84 | 183.70 | 7.07 | 230.23 | 0.1579 | -492.0 | -427.3 | |
| 0.00 | 2.13 | 0.00 | 1.07 | -11.35 | 183.59 | 6.96 | 227.31 | 0.1623 | 546.0 | 540.7 | |
| 0.00 | 1.86 | 0.00 | 0.93 | -6.86 | 183.44 | 6.81 | 255.17 | 0.1224 | -808.0 | -622.8 | |
| 0.00 | 1.60 | 0.00 | 0.80 | -10.81 | 183.42 | 6.79 | 229.25 | 0.1540 | -1014.0 | -917.4 | |
| 0.00 | 6.30 | 0.00 | 3.15 | -7.70 | 183.36 | 6.73 | 248.44 | 0.1255 | -946.0 | -804.5 | |
| 0.00 | 1.78 | 0.00 | 0.89 | -10.02 | 183.37 | 6.74 | 233.23 | 0.1450 | -868.0 | -633.2 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -9.63 | 183.24 | 6.61 | 234.98 | 0.1392 | -798.0 | -657.4 | |
| 0.00 | 1.78 | 0.00 | 0.89 | -9.51 | 183.09 | 6.46 | 235.07 | 0.1359 | -1139.0 | -911.0 | |
| 0.80 | 2.22 | 0.40 | 1.11 | -10.12 | 183.07 | 6.44 | 231.44 | 0.1417 | -1095.9 | -856.6 | |
| 0.00 | 1.60 | 0.00 | 0.80 | -9.76 | 183.00 | 6.37 | 233.24 | 0.1370 | -1158.0 | -840.6 | |
| 0.00 | 1.07 | 0.00 | 0.53 | -8.82 | 182.98 | 6.35 | 239.13 | 0.1279 | -856.0 | -732.9 | |
| 1.86 | 3.11 | 0.93 | 1.55 | -7.68 | 182.72 | 6.09 | 246.66 | 0.1150 | -1108.3 | -869.1 | |
| 17.75 | 58.32 | 8.92 | 29.30 | -12.61 | 182.62 | 5.99 | 217.86 | 0.1667 | 1311.6 | 555.9 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -7.50 | 182.53 | 5.90 | 247.52 | 0.1109 | -989.0 | -765.3 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -13.28 | 182.33 | 5.70 | 214.12 | 0.1730 | 674.0 | 446.8 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -9.97 | 182.02 | 5.39 | 227.31 | 0.1264 | -862.0 | -832.0 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -15.20 | 181.72 | 5.08 | 205.96 | 0.1963 | -921.0 | -833.4 | |
| 0.00 | 1.60 | 0.00 | 0.80 | -8.71 | 181.54 | 4.91 | 233.24 | 0.1061 | 923.0 | 662.9 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -13.77 | 181.59 | 4.96 | 209.08 | 0.1736 | 729.0 | 600.1 | |
| 0.00 | 2.31 | 0.00 | 1.15 | -9.77 | 181.31 | 4.68 | 224.57 | 0.1151 | -709.0 | -680.2 | |
| 0.00 | 1.78 | 0.00 | 0.90 | -14.87 | 181.33 | 4.70 | 205.00 | 0.1883 | -800.0 | -489.0 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -12.10 | 180.42 | 3.79 | 207.88 | 0.1387 | -744.0 | -536.7 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -16.32 | 180.39 | 3.76 | 197.91 | 0.2055 | 914.0 | 670.5 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -13.63 | 179.32 | 2.69 | 197.09 | 0.1559 | -597.0 | -409.7 | |
| 0.00 | 2.49 | 0.00 | 1.26 | -18.11 | 178.01 | 1.38 | 185.81 | 0.2272 | 1043.0 | 882.9 | |
| 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. | |