SDO HMI 2014-04-23 23:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.46 | 0.00 | 9.80 | -10.89 | 139.02 | -1.83 | 160.56 | 0.1705 | 692.6 | 546.8 | |
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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 | 2.31 | 0.00 | 1.17 | -11.83 | 150.83 | 9.98 | 234.24 | 0.2100 | 789.0 | 697.5 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -15.44 | 149.94 | 9.09 | 219.57 | 0.2401 | 750.0 | 600.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -7.73 | 145.75 | 4.89 | 239.38 | 0.0987 | 737.0 | 591.4 | |
| 0.00 | 2.13 | 0.00 | 1.06 | -11.16 | 142.13 | 1.28 | 191.32 | 0.1121 | 749.0 | 595.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -12.89 | 139.76 | -1.10 | 172.38 | 0.1412 | 836.0 | 487.3 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -14.56 | 137.78 | -3.07 | 162.88 | 0.1768 | -944.0 | -761.6 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -15.38 | 137.05 | -3.80 | 160.68 | 0.1941 | 1095.0 | 838.7 | |
| 0.00 | 1.60 | 0.00 | 0.81 | -15.19 | 136.96 | -3.89 | 159.93 | 0.1917 | 924.0 | 664.9 | |
| 0.00 | 1.60 | 0.00 | 0.81 | -14.70 | 136.56 | -4.29 | 157.05 | 0.1863 | 838.0 | 572.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -9.84 | 136.47 | -4.39 | 138.98 | 0.1154 | 889.0 | 739.3 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -10.02 | 136.31 | -4.54 | 139.02 | 0.1195 | 792.0 | 641.4 | |
| 0.00 | 1.87 | 0.00 | 0.93 | -2.27 | 133.53 | -7.32 | 70.57 | 0.1356 | 754.0 | 563.3 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 0.29 | 128.46 | -12.39 | 67.67 | 0.2330 | 750.0 | 612.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -9.20 | 127.72 | -13.13 | 109.08 | 0.2383 | 738.0 | 582.1 | |
| 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. | |