SDO HMI 2014-05-30 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.71 | 100.85 | 14.77 | 51.78 | -9.08 | 24.86 | 12.71 | 235.91 | 0.2631 | 645.5 | 493.9 | |
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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 | 0.90 | 0.00 | 0.47 | -6.92 | 26.97 | 14.82 | 247.24 | 0.2767 | 844.0 | 665.6 | |
| 5.87 | 19.05 | 3.03 | 9.83 | -8.79 | 26.31 | 14.16 | 240.12 | 0.2800 | 1042.9 | 748.2 | |
| 3.61 | 62.21 | 1.86 | 31.98 | -9.32 | 25.54 | 13.39 | 237.09 | 0.2734 | 843.5 | 538.3 | |
| 17.79 | -3.00 | 9.14 | -3.00 | -8.98 | 25.40 | 13.25 | 237.89 | 0.2684 | 1246.4 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.15 | -9.69 | 23.53 | 11.38 | 231.60 | 0.2493 | 968.0 | 702.9 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -9.78 | 23.19 | 11.04 | 230.46 | 0.2458 | 1010.0 | 868.8 | |
| 0.00 | 2.71 | 0.00 | 1.39 | -10.21 | 23.11 | 10.96 | 228.90 | 0.2494 | 886.0 | 741.3 | |
| 1.44 | 3.16 | 0.74 | 1.61 | -10.03 | 22.88 | 10.73 | 228.89 | 0.2445 | 1127.1 | 899.1 | |
| 0.00 | 1.72 | 0.00 | 0.87 | -8.92 | 22.32 | 10.17 | 231.06 | 0.2252 | 823.0 | 614.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -8.43 | 20.47 | 8.32 | 227.23 | 0.1958 | -929.0 | -691.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -8.43 | 20.10 | 7.95 | 225.93 | 0.1912 | -759.0 | -673.8 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -9.41 | 20.02 | 7.87 | 222.14 | 0.2023 | -802.0 | -561.1 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -8.62 | 20.01 | 7.86 | 224.92 | 0.1923 | -819.0 | -679.7 | |
| 0.00 | 1.63 | 0.00 | 0.82 | -10.34 | 17.06 | 4.91 | 207.02 | 0.1863 | -799.0 | -624.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | -10.80 | 13.78 | 1.63 | 189.20 | 0.1761 | -744.0 | -715.2 | |
| 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. | |