SDO HMI 2012-05-07 02:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.94 | 42.68 | 4.78 | 23.41 | 16.06 | 225.96 | -16.01 | 38.19 | 0.4272 | 71.4 | 224.1 | |
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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 | 1.61 | 0.00 | 0.87 | 18.11 | 231.57 | -10.39 | 25.02 | 0.4072 | -763.0 | -436.9 | |
| 7.87 | 15.03 | 4.18 | 7.99 | 13.61 | 229.36 | -12.60 | 35.90 | 0.3632 | -1028.6 | -786.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 13.88 | 228.19 | -13.77 | 37.87 | 0.3781 | -728.0 | -567.1 | |
| 0.00 | 1.34 | 0.00 | 0.75 | 18.62 | 225.56 | -16.40 | 35.56 | 0.4620 | -744.0 | -576.7 | |
| 0.00 | 1.88 | 0.00 | 1.03 | 16.17 | 225.20 | -16.77 | 39.66 | 0.4359 | 819.0 | 648.2 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 16.98 | 224.63 | -17.34 | 39.37 | 0.4512 | 792.0 | 728.6 | |
| 0.00 | 5.37 | 0.00 | 2.98 | 17.24 | 224.54 | -17.43 | 39.13 | 0.4551 | 681.0 | 679.0 | |
| 1.07 | 2.06 | 0.60 | 1.15 | 17.28 | 224.17 | -17.80 | 39.65 | 0.4592 | 717.2 | 703.7 | |
| 0.00 | 1.70 | 0.00 | 0.96 | 17.73 | 223.05 | -18.91 | 40.70 | 0.4755 | 699.0 | 614.9 | |
| 0.00 | 2.68 | 0.00 | 1.51 | 17.34 | 222.79 | -19.17 | 41.64 | 0.4738 | 825.0 | 724.5 | |
| 0.00 | 2.77 | 0.00 | 1.57 | 17.93 | 222.69 | -19.27 | 40.93 | 0.4813 | 643.0 | 578.4 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 17.12 | 222.65 | -19.32 | 42.18 | 0.4728 | 685.0 | 598.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 16.83 | 222.68 | -19.29 | 42.57 | 0.4693 | 722.0 | 569.4 | |
| 0.00 | 2.06 | 0.00 | 1.16 | 17.74 | 222.51 | -19.45 | 41.46 | 0.4810 | 669.0 | 548.0 | |
| 0.00 | 2.60 | 0.00 | 1.46 | 17.45 | 222.51 | -19.46 | 41.89 | 0.4778 | 839.0 | 633.5 | |
| 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. | |