SDO HMI 2011-05-03 04:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.43 | 315.22 | 26.73 | 182.15 | 17.61 | 62.07 | -22.45 | 45.02 | 0.5162 | -739.4 | -329.3 | |
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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 |
| 1.07 | 299.33 | 0.61 | 172.36 | 17.06 | 62.82 | -21.70 | 44.92 | 0.5026 | -1194.2 | -388.5 | |
| 45.36 | -1.00 | 26.12 | -1.00 | 17.55 | 62.42 | -22.10 | 44.72 | 0.5119 | -1267.1 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.47 | 17.65 | 59.22 | -25.31 | 48.34 | 0.5473 | -573.0 | -471.1 | |
| 0.00 | 1.16 | 0.00 | 0.70 | 18.32 | 57.44 | -27.08 | 49.25 | 0.5727 | 666.0 | 538.8 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 18.31 | 56.80 | -27.73 | 49.90 | 0.5796 | 789.0 | 654.4 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 18.71 | 56.54 | -27.98 | 49.59 | 0.5857 | 593.0 | 610.1 | |
| 0.00 | 0.54 | 0.00 | 0.34 | 22.53 | 55.62 | -28.91 | 45.52 | 0.6280 | 245.0 | 167.8 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 19.38 | 56.09 | -28.43 | 49.11 | 0.5962 | 607.0 | 551.0 | |
| 0.00 | 0.80 | 0.00 | 0.49 | 18.40 | 56.20 | -28.32 | 50.35 | 0.5868 | 642.0 | 540.3 | |
| 0.00 | 3.66 | 0.00 | 2.22 | 17.32 | 56.32 | -28.20 | 51.76 | 0.5766 | 798.0 | 663.8 | |
| 0.00 | 1.25 | 0.00 | 0.77 | 19.43 | 55.83 | -28.69 | 49.31 | 0.5994 | 606.0 | 504.6 | |
| 0.00 | 1.43 | 0.00 | 0.93 | 23.16 | 53.95 | -30.57 | 46.26 | 0.6495 | 649.0 | 569.1 | |
| 0.00 | 3.13 | 0.00 | 1.96 | 18.20 | 53.64 | -30.88 | 52.94 | 0.6133 | 905.0 | 704.2 | |
| 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. | |