SDO HMI 2014-05-29 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.23 | 50.37 | 10.87 | 28.18 | -19.61 | 51.12 | 20.75 | 225.84 | 0.4664 | 308.3 | -37.5 | |
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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 | 0.90 | 0.00 | 0.51 | -18.79 | 54.01 | 23.64 | 231.02 | 0.4903 | 793.0 | 694.7 | |
| 15.44 | 22.12 | 8.78 | 12.57 | -19.34 | 53.81 | 23.44 | 229.89 | 0.4928 | 966.6 | 674.7 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -14.78 | 53.11 | 22.75 | 237.32 | 0.4460 | 668.0 | 613.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -18.44 | 53.50 | 23.14 | 231.04 | 0.4813 | 718.0 | 581.0 | |
| 0.00 | 1.99 | 0.00 | 1.11 | -19.35 | 50.86 | 20.49 | 226.25 | 0.4591 | -728.0 | -602.5 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -20.64 | 50.86 | 20.49 | 224.16 | 0.4722 | 722.0 | 566.4 | |
| 0.00 | 2.98 | 0.00 | 1.67 | -20.28 | 50.57 | 20.20 | 224.33 | 0.4654 | 404.0 | 393.7 | |
| 3.79 | 11.74 | 2.09 | 6.46 | -19.81 | 48.59 | 18.22 | 222.28 | 0.4391 | -1017.1 | -786.7 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -22.24 | 48.45 | 18.08 | 218.33 | 0.4650 | 604.0 | 508.6 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -20.98 | 46.72 | 16.35 | 217.50 | 0.4336 | -202.0 | -162.6 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -19.66 | 46.34 | 15.97 | 218.93 | 0.4141 | -871.0 | -649.9 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -19.79 | 45.92 | 15.55 | 218.00 | 0.4115 | -898.0 | -744.4 | |
| 0.00 | 2.17 | 0.00 | 1.17 | -21.86 | 42.36 | 11.99 | 208.39 | 0.4073 | -829.0 | -667.0 | |
| 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. | |