SDO HMI 2014-05-16 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.33 | 32.19 | 1.69 | 16.36 | 8.26 | 196.14 | -7.31 | 33.22 | 0.2278 | -63.1 | -47.4 | |
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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 | 1.35 | 0.00 | 0.68 | 6.17 | 198.93 | -4.51 | 27.40 | 0.1708 | -792.0 | -565.1 | |
| 2.25 | 4.22 | 1.14 | 2.14 | 8.18 | 198.46 | -4.99 | 24.93 | 0.2053 | -1145.8 | -866.5 | |
| 0.00 | 2.43 | 0.00 | 1.22 | 6.85 | 198.44 | -5.01 | 28.07 | 0.1851 | -703.0 | -682.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 7.16 | 198.38 | -5.07 | 27.60 | 0.1903 | -876.0 | -696.1 | |
| 1.08 | 5.12 | 0.55 | 2.60 | 8.46 | 197.62 | -5.83 | 27.84 | 0.2160 | -1147.9 | -875.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 8.80 | 197.59 | -5.86 | 27.26 | 0.2214 | -724.0 | -598.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 8.43 | 197.28 | -6.17 | 29.26 | 0.2183 | -927.0 | -680.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 8.50 | 196.48 | -6.97 | 32.18 | 0.2263 | -889.0 | -707.2 | |
| 0.00 | 2.16 | 0.00 | 1.10 | 7.09 | 194.84 | -8.61 | 41.77 | 0.2241 | 766.0 | 754.1 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 10.06 | 194.37 | -9.08 | 35.59 | 0.2682 | 710.0 | 478.3 | |
| 0.00 | 4.58 | 0.00 | 2.35 | 9.38 | 193.95 | -9.50 | 38.38 | 0.2634 | 957.0 | 799.1 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 8.55 | 193.35 | -10.10 | 42.20 | 0.2593 | 910.0 | 848.7 | |
| 0.00 | 2.43 | 0.00 | 1.24 | 8.43 | 193.17 | -10.28 | 43.03 | 0.2599 | 861.0 | 673.4 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.68 | 193.10 | -10.35 | 42.57 | 0.2638 | 862.0 | 761.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 8.75 | 191.94 | -11.51 | 45.40 | 0.2782 | 856.0 | 535.5 | |
| 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. | |