SDO HMI 2014-05-16 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.51 | 43.32 | 5.37 | 22.09 | -15.46 | 193.88 | -5.16 | 158.86 | 0.2422 | 366.1 | 459.5 | |
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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 |
| 4.85 | 6.82 | 2.48 | 3.49 | -16.44 | 195.03 | -4.00 | 164.46 | 0.2512 | 1117.3 | 789.3 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -16.09 | 195.04 | -4.00 | 164.10 | 0.2456 | 916.0 | 672.8 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.07 | 194.96 | -4.07 | 162.52 | 0.2292 | 863.0 | 689.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -12.84 | 194.85 | -4.18 | 158.39 | 0.1941 | -731.0 | -417.9 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -15.22 | 194.68 | -4.36 | 161.60 | 0.2332 | 767.0 | 512.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -15.65 | 194.60 | -4.43 | 161.91 | 0.2406 | 886.0 | 742.4 | |
| 0.54 | 1.53 | 0.27 | 0.77 | -12.53 | 194.54 | -4.49 | 156.33 | 0.1912 | -981.0 | -810.3 | |
| 0.00 | 4.94 | 0.00 | 2.53 | -16.46 | 194.43 | -4.61 | 162.31 | 0.2546 | 741.0 | 555.7 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -15.06 | 193.83 | -5.20 | 158.08 | 0.2357 | 1066.0 | 873.5 | |
| 0.00 | 2.07 | 0.00 | 1.05 | -15.09 | 193.64 | -5.39 | 157.42 | 0.2374 | 957.0 | 768.0 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -15.56 | 193.63 | -5.41 | 158.13 | 0.2447 | 521.0 | 73.8 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -14.84 | 193.58 | -5.45 | 156.78 | 0.2339 | 692.0 | 551.9 | |
| 1.35 | 10.96 | 0.69 | 5.59 | -15.27 | 193.26 | -5.78 | 156.31 | 0.2428 | 1042.0 | 798.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -15.83 | 193.24 | -5.79 | 157.19 | 0.2516 | -573.0 | -378.3 | |
| 3.77 | 6.02 | 1.93 | 3.08 | -15.39 | 192.43 | -6.60 | 153.62 | 0.2506 | -1031.2 | -764.1 | |
| 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. | |