SDO HMI 2014-05-28 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.62 | 164.79 | 15.58 | 89.87 | -8.86 | 24.86 | -23.67 | 108.92 | 0.4211 | 836.0 | 446.3 | |
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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 |
| 23.65 | 140.71 | 12.85 | 76.45 | -8.81 | 25.37 | -23.16 | 109.15 | 0.4132 | 1262.4 | 456.4 | |
| 2.26 | -1.00 | 1.23 | -1.00 | -8.81 | 24.97 | -23.57 | 108.86 | 0.4193 | 854.0 | 999999 | |
| 0.90 | -1.00 | 0.49 | -1.00 | -8.81 | 24.73 | -23.80 | 108.70 | 0.4228 | 786.6 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -8.10 | 24.61 | -23.92 | 107.00 | 0.4215 | 705.0 | 472.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -8.22 | 24.20 | -24.33 | 107.02 | 0.4283 | 570.0 | 387.1 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -7.94 | 24.22 | -24.32 | 106.41 | 0.4269 | 749.0 | 628.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -8.77 | 23.82 | -24.71 | 108.02 | 0.4363 | 788.0 | 640.7 | |
| 0.00 | 2.89 | 0.00 | 1.59 | -8.27 | 23.59 | -24.95 | 106.79 | 0.4378 | 714.0 | 587.0 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -9.31 | 22.93 | -25.60 | 108.65 | 0.4519 | 672.0 | 592.7 | |
| 1.81 | 11.46 | 1.01 | 6.39 | -9.58 | 22.26 | -26.28 | 108.81 | 0.4630 | 972.5 | 706.5 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -9.50 | 19.80 | -28.74 | 107.29 | 0.4986 | -805.0 | -542.4 | |
| 0.00 | 1.90 | 0.00 | 1.08 | -9.68 | 19.74 | -28.79 | 107.62 | 0.5001 | -793.0 | -622.1 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -8.76 | 19.83 | -28.71 | 105.86 | 0.4955 | -641.0 | -591.6 | |
| 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. | |