SDO HMI 2014-10-08 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.26 | 0.00 | 11.69 | -18.77 | 101.27 | 16.58 | 212.15 | 0.5100 | -58.4 | -52.5 | |
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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 | 1.49 | 0.00 | 0.88 | -13.81 | 110.69 | 26.01 | 231.96 | 0.5428 | 738.0 | 678.9 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -13.35 | 110.47 | 25.78 | 232.41 | 0.5362 | 873.0 | 725.6 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -22.67 | 108.35 | 23.66 | 217.89 | 0.6053 | 795.0 | 666.0 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -22.56 | 108.18 | 23.50 | 217.82 | 0.6027 | 741.0 | 652.8 | |
| 0.00 | 1.49 | 0.00 | 0.92 | -23.46 | 107.11 | 22.42 | 215.59 | 0.6035 | 637.0 | 523.4 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -23.84 | 107.00 | 22.31 | 215.07 | 0.6067 | 590.0 | 496.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -16.94 | 102.02 | 17.34 | 216.17 | 0.4850 | -759.0 | -641.4 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -7.59 | 100.40 | 15.71 | 228.66 | 0.3591 | 730.0 | 503.3 | |
| 0.00 | 2.02 | 0.00 | 1.14 | -18.37 | 99.96 | 15.27 | 211.13 | 0.4855 | -737.0 | -554.8 | |
| 0.00 | 1.40 | 0.00 | 0.80 | -18.98 | 99.46 | 14.77 | 209.63 | 0.4896 | -778.0 | -614.1 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -19.34 | 97.99 | 13.30 | 206.78 | 0.4837 | -599.0 | -400.7 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -19.14 | 97.97 | 13.28 | 206.95 | 0.4809 | -810.0 | -600.4 | |
| 0.00 | 1.58 | 0.00 | 0.90 | -22.27 | 93.96 | 9.27 | 197.35 | 0.5018 | -752.0 | -549.6 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -19.42 | 92.91 | 8.23 | 197.31 | 0.4555 | -766.0 | -650.9 | |
| 0.00 | 1.84 | 0.00 | 1.02 | -19.77 | 89.09 | 4.40 | 189.34 | 0.4470 | -779.0 | -501.2 | |
| 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. | |