SDO HMI 2014-05-28 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.37 | 89.61 | 19.09 | 47.06 | -19.32 | 50.87 | 6.18 | 198.03 | 0.3318 | 172.7 | 408.0 | |
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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 | 2.80 | 0.00 | 1.47 | -18.58 | 52.33 | 7.64 | 202.75 | 0.3272 | 1001.0 | 838.6 | |
| 19.13 | 45.49 | 10.05 | 23.91 | -19.09 | 52.19 | 7.50 | 201.76 | 0.3340 | 1120.5 | 742.7 | |
| 0.00 | 3.97 | 0.00 | 2.08 | -19.16 | 51.68 | 6.98 | 200.32 | 0.3320 | 1039.0 | 675.7 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -19.76 | 51.57 | 6.88 | 199.40 | 0.3407 | 441.0 | 493.2 | |
| 0.00 | 2.17 | 0.00 | 1.12 | -16.96 | 50.44 | 5.75 | 199.31 | 0.2909 | 789.0 | 563.5 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -17.12 | 50.45 | 5.75 | 199.13 | 0.2934 | 877.0 | 646.8 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -20.99 | 50.55 | 5.85 | 195.63 | 0.3547 | 859.0 | 784.8 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -19.99 | 50.45 | 5.75 | 196.21 | 0.3386 | 812.0 | 546.4 | |
| 1.90 | 27.26 | 0.99 | 14.29 | -19.38 | 49.42 | 4.72 | 193.91 | 0.3245 | -1109.5 | -542.0 | |
| 15.34 | -9.00 | 8.05 | -9.00 | -19.73 | 49.37 | 4.67 | 193.49 | 0.3299 | -1071.5 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -20.34 | 45.04 | 0.34 | 180.97 | 0.3309 | -858.0 | -614.2 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -22.38 | 42.58 | -2.12 | 174.61 | 0.3660 | -794.0 | -615.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -22.51 | 41.16 | -3.54 | 171.11 | 0.3709 | -678.0 | -551.7 | |
| 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. | |