SDO HMI 2014-09-28 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.98 | 0.00 | 11.30 | 6.83 | 207.86 | -15.35 | 89.34 | 0.2644 | -26.0 | -18.4 | |
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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 | 1.06 | 0.00 | 0.54 | 7.76 | 210.39 | -12.82 | 85.20 | 0.2217 | -777.0 | -581.9 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 6.34 | 210.30 | -12.91 | 91.59 | 0.2232 | -867.0 | -667.0 | |
| 0.00 | 4.24 | 0.00 | 2.16 | 6.47 | 209.46 | -13.75 | 90.85 | 0.2373 | -880.0 | -564.2 | |
| 0.00 | 1.68 | 0.00 | 0.86 | 6.31 | 209.25 | -13.97 | 91.46 | 0.2411 | -893.0 | -769.1 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 6.63 | 208.65 | -14.57 | 90.08 | 0.2510 | -900.0 | -682.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 6.58 | 208.08 | -15.13 | 90.19 | 0.2605 | -832.0 | -673.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 6.75 | 207.70 | -15.51 | 89.51 | 0.2668 | -779.0 | -536.1 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 5.69 | 207.51 | -15.70 | 93.41 | 0.2710 | 852.0 | 698.2 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 6.06 | 206.65 | -16.56 | 91.86 | 0.2848 | 847.0 | 644.6 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 6.57 | 206.64 | -16.58 | 90.06 | 0.2847 | 825.0 | 619.3 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 7.17 | 206.59 | -16.63 | 87.95 | 0.2854 | 710.0 | 585.8 | |
| 0.00 | 1.85 | 0.00 | 0.96 | 5.81 | 206.50 | -16.71 | 92.69 | 0.2877 | 719.0 | 568.6 | |
| 0.00 | 2.38 | 0.00 | 1.24 | 8.31 | 205.87 | -17.34 | 84.07 | 0.2978 | 869.0 | 749.1 | |
| 0.00 | 1.85 | 0.00 | 0.96 | 8.52 | 205.77 | -17.45 | 83.40 | 0.2998 | 742.0 | 613.1 | |
| 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. | |