SDO HMI 2011-10-26 09:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.86 | 41.88 | 4.13 | 25.23 | 14.98 | 241.56 | -33.77 | 70.64 | 0.5713 | 277.2 | 70.2 | |
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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 | 1.22 | 0.00 | 0.71 | 15.26 | 245.13 | -30.21 | 68.60 | 0.5235 | -853.0 | -666.4 | |
| 1.39 | 3.30 | 0.81 | 1.92 | 15.31 | 244.83 | -30.51 | 68.66 | 0.5278 | -669.9 | -596.8 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 15.37 | 243.48 | -31.85 | 69.19 | 0.5465 | -388.0 | -326.5 | |
| 0.00 | 1.30 | 0.00 | 0.77 | 14.09 | 242.78 | -32.55 | 71.75 | 0.5517 | 650.0 | 497.3 | |
| 0.00 | 2.00 | 0.00 | 1.19 | 15.23 | 242.48 | -32.86 | 69.87 | 0.5597 | -522.0 | -421.2 | |
| 0.00 | 9.29 | 0.00 | 5.62 | 16.41 | 241.59 | -33.75 | 68.24 | 0.5760 | -754.0 | -718.3 | |
| 0.00 | 1.22 | 0.00 | 0.73 | 14.21 | 241.29 | -34.05 | 72.11 | 0.5725 | 863.0 | 713.8 | |
| 0.00 | 4.17 | 0.00 | 2.52 | 14.35 | 241.15 | -34.18 | 71.91 | 0.5748 | 627.0 | 631.5 | |
| 0.00 | 2.35 | 0.00 | 1.42 | 14.08 | 241.05 | -34.29 | 72.42 | 0.5754 | 711.0 | 644.3 | |
| 3.91 | 12.16 | 2.37 | 7.39 | 14.30 | 240.71 | -34.62 | 72.15 | 0.5806 | 872.4 | 644.9 | |
| 1.56 | -10.00 | 0.95 | -10.00 | 14.41 | 240.51 | -34.83 | 72.03 | 0.5838 | 758.2 | 999999 | |
| 0.00 | 2.69 | 0.00 | 1.65 | 14.75 | 239.99 | -35.35 | 71.64 | 0.5917 | 764.0 | 629.5 | |
| 0.00 | 0.96 | 0.00 | 0.59 | 14.89 | 239.74 | -35.60 | 71.50 | 0.5955 | 573.0 | 534.2 | |
| 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. | |