SDO HMI 2014-05-16 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.10 | 46.00 | 3.64 | 23.66 | 8.53 | 195.97 | -10.76 | 43.59 | 0.2678 | -187.8 | -87.7 | |
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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 |
| 5.21 | 8.89 | 2.66 | 4.54 | 8.16 | 198.26 | -8.48 | 38.22 | 0.2370 | -1111.6 | -728.0 | |
| 0.00 | 1.98 | 0.00 | 1.00 | 6.72 | 198.01 | -8.73 | 43.20 | 0.2212 | -932.0 | -712.6 | |
| 0.00 | 3.59 | 0.00 | 1.84 | 8.75 | 197.72 | -9.02 | 38.41 | 0.2505 | -880.0 | -718.8 | |
| 0.00 | 5.93 | 0.00 | 3.03 | 8.51 | 197.38 | -9.35 | 40.06 | 0.2509 | -1072.0 | -854.2 | |
| 0.00 | 1.98 | 0.00 | 1.01 | 8.30 | 196.95 | -9.78 | 41.89 | 0.2530 | -938.0 | -845.3 | |
| 0.00 | 4.31 | 0.00 | 2.22 | 8.52 | 196.01 | -10.72 | 43.90 | 0.2666 | -786.0 | -666.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 8.38 | 194.89 | -11.84 | 47.11 | 0.2784 | -866.0 | -706.1 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 7.39 | 194.86 | -11.88 | 49.94 | 0.2679 | 822.0 | 682.6 | |
| 0.99 | 3.68 | 0.51 | 1.91 | 9.31 | 194.20 | -12.53 | 46.32 | 0.2974 | 1060.2 | 967.1 | |
| 0.00 | 4.04 | 0.00 | 2.10 | 9.38 | 193.95 | -12.79 | 46.73 | 0.3012 | 944.0 | 813.6 | |
| 0.00 | 2.79 | 0.00 | 1.45 | 9.38 | 193.69 | -13.04 | 47.28 | 0.3043 | 872.0 | 680.8 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 8.39 | 193.54 | -13.19 | 50.13 | 0.2955 | 894.0 | 765.8 | |
| 0.90 | 4.76 | 0.47 | 2.47 | 8.52 | 193.25 | -13.48 | 50.40 | 0.3006 | 1094.7 | 871.9 | |
| 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. | |