SDO HMI 2011-05-06 03:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.32 | 301.89 | 22.87 | 167.18 | 18.11 | 60.76 | 15.34 | 325.74 | 0.4493 | -721.3 | -391.8 | |
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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 | 1.16 | 0.00 | 0.67 | 22.81 | 62.64 | 17.22 | 328.39 | 0.5227 | -715.0 | -488.2 | |
| 36.22 | 284.82 | 20.05 | 157.68 | 17.88 | 61.12 | 15.70 | 324.81 | 0.4488 | -1348.1 | -438.9 | |
| 5.10 | -2.00 | 2.82 | -2.00 | 18.20 | 60.78 | 15.37 | 325.81 | 0.4498 | -1011.8 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 19.35 | 59.07 | 13.65 | 330.24 | 0.4505 | -715.0 | -550.6 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 19.27 | 58.54 | 13.12 | 331.12 | 0.4455 | -643.0 | -481.5 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 26.14 | 58.92 | 13.50 | 337.08 | 0.5403 | -754.0 | -604.4 | |
| 0.00 | 1.70 | 0.00 | 0.93 | 18.31 | 57.90 | 12.49 | 331.18 | 0.4277 | 770.0 | 620.3 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 19.66 | 55.55 | 10.13 | 337.26 | 0.4304 | 664.0 | 527.1 | |
| 0.00 | 0.89 | 0.00 | 0.51 | 23.34 | 55.78 | 10.36 | 339.98 | 0.4845 | 697.0 | 610.6 | |
| 0.00 | 1.16 | 0.00 | 0.66 | 23.85 | 55.45 | 10.04 | 340.94 | 0.4901 | 733.0 | 578.9 | |
| 0.00 | 1.34 | 0.00 | 0.76 | 23.97 | 54.52 | 9.11 | 342.67 | 0.4875 | 716.0 | 558.3 | |
| 0.00 | 2.24 | 0.00 | 1.21 | 18.66 | 53.93 | 8.52 | 339.70 | 0.4063 | 891.0 | 669.6 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 21.67 | 49.78 | 4.36 | 350.62 | 0.4356 | 819.0 | 616.5 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 21.60 | 49.42 | 4.00 | 351.36 | 0.4337 | 834.0 | 674.4 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 21.73 | 49.29 | 3.87 | 351.68 | 0.4355 | 712.0 | 528.4 | |
| 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. | |