SDO HMI 2011-05-02 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 |
| 2.77 | 22.48 | 1.55 | 12.51 | -18.22 | 121.82 | 23.53 | 236.51 | 0.4568 | -254.9 | -162.6 | |
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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 |
| 1.61 | 3.66 | 0.90 | 2.06 | -17.00 | 124.08 | 25.79 | 241.06 | 0.4774 | 848.1 | 669.5 | |
| 0.00 | 2.41 | 0.00 | 1.36 | -17.35 | 123.78 | 25.49 | 240.14 | 0.4757 | 889.0 | 720.6 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -16.80 | 123.42 | 25.13 | 240.89 | 0.4673 | 835.0 | 706.1 | |
| 0.00 | 1.61 | 0.00 | 0.90 | -17.48 | 123.49 | 25.20 | 239.63 | 0.4726 | 616.0 | 518.0 | |
| 1.16 | 1.52 | 0.65 | 0.85 | -17.11 | 123.40 | 25.11 | 240.26 | 0.4690 | 898.2 | 768.8 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -18.36 | 121.14 | 22.86 | 235.68 | 0.4482 | -734.0 | -560.6 | |
| 0.00 | 1.34 | 0.00 | 0.74 | -19.28 | 120.69 | 22.40 | 233.41 | 0.4498 | -852.0 | -639.5 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -19.72 | 120.75 | 22.46 | 232.66 | 0.4542 | -563.0 | -456.8 | |
| 0.00 | 1.87 | 0.00 | 1.03 | -18.23 | 120.16 | 21.87 | 234.86 | 0.4345 | -932.0 | -779.8 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -19.85 | 120.39 | 22.10 | 232.00 | 0.4509 | -855.0 | -685.4 | |
| 0.00 | 3.12 | 0.00 | 1.72 | -19.20 | 120.22 | 21.94 | 233.05 | 0.4433 | -913.0 | -753.0 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -18.49 | 119.99 | 21.70 | 234.16 | 0.4344 | -858.0 | -704.0 | |
| 0.00 | 1.34 | 0.00 | 0.74 | -19.34 | 119.59 | 21.30 | 232.03 | 0.4366 | -693.0 | -569.7 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -19.23 | 119.16 | 20.87 | 231.73 | 0.4303 | -741.0 | -494.5 | |
| 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. | |