SDO HMI 2014-04-06 12:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.97 | 25.43 | 0.48 | 12.66 | -8.27 | 7.56 | -3.83 | 136.85 | 0.0912 | -12.6 | -149.5 | |
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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 | 3.34 | 0.00 | 1.66 | -8.29 | 12.64 | 1.26 | 210.97 | 0.0423 | 769.0 | 738.9 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -8.44 | 12.40 | 1.01 | 204.30 | 0.0427 | 874.0 | 723.2 | |
| 0.00 | 1.32 | 0.00 | 0.65 | -8.95 | 12.31 | 0.92 | 198.47 | 0.0504 | 972.0 | 762.2 | |
| 0.00 | 1.41 | 0.00 | 0.70 | -10.06 | 10.36 | -1.03 | 165.26 | 0.0695 | 1042.0 | 809.2 | |
| 0.97 | 1.67 | 0.48 | 0.83 | -9.69 | 10.09 | -1.30 | 159.80 | 0.0649 | 1033.9 | 942.8 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -9.12 | 9.82 | -1.57 | 151.96 | 0.0577 | 887.0 | 678.7 | |
| 0.00 | 1.41 | 0.00 | 0.70 | -7.38 | 5.53 | -5.86 | 101.60 | 0.1039 | -1012.0 | -796.1 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -6.96 | 5.38 | -6.01 | 97.38 | 0.1053 | -1198.0 | -1000.8 | |
| 0.00 | 2.90 | 0.00 | 1.45 | -7.40 | 5.25 | -6.14 | 101.36 | 0.1086 | -969.0 | -768.1 | |
| 0.00 | 2.38 | 0.00 | 1.18 | -7.34 | 4.98 | -6.41 | 100.37 | 0.1131 | -1031.0 | -824.4 | |
| 0.00 | 3.26 | 0.00 | 1.62 | -7.58 | 4.94 | -6.44 | 102.39 | 0.1144 | -1034.0 | -869.8 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -7.45 | 4.46 | -6.93 | 100.58 | 0.1223 | -844.0 | -725.1 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -12.25 | 3.48 | -7.90 | 128.28 | 0.1720 | 790.0 | 600.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -7.77 | 3.39 | -8.00 | 101.50 | 0.1414 | -958.0 | -755.8 | |
| 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. | |