SDO HMI 2014-12-10 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.50 | 0.00 | 10.19 | 15.77 | 15.77 | 37.88 | 295.38 | 0.6556 | -386.9 | -364.6 | |
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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 | 1.19 | 0.00 | 0.82 | 12.84 | 20.23 | 42.34 | 288.98 | 0.6968 | -625.0 | -560.6 | |
| 0.00 | 1.02 | 0.00 | 0.70 | 14.78 | 18.95 | 41.05 | 292.18 | 0.6881 | -365.0 | -421.9 | |
| 0.00 | 3.15 | 0.00 | 2.18 | 16.79 | 19.28 | 41.39 | 294.79 | 0.6997 | -621.0 | -499.2 | |
| 0.00 | 0.43 | 0.00 | 0.29 | 14.75 | 18.61 | 40.72 | 292.27 | 0.6841 | -534.0 | -508.8 | |
| 0.00 | 0.77 | 0.00 | 0.52 | 15.83 | 18.06 | 40.17 | 294.01 | 0.6817 | -547.0 | -408.9 | |
| 0.00 | 0.85 | 0.00 | 0.58 | 17.46 | 18.48 | 40.59 | 296.08 | 0.6934 | -544.0 | -494.8 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 11.14 | 17.00 | 39.10 | 287.65 | 0.6518 | -674.0 | -610.7 | |
| 0.00 | 0.60 | 0.00 | 0.39 | 11.16 | 16.81 | 38.92 | 287.77 | 0.6495 | -505.0 | -556.0 | |
| 0.00 | 0.34 | 0.00 | 0.23 | 15.73 | 16.96 | 39.07 | 294.37 | 0.6683 | -512.0 | -556.5 | |
| 0.00 | 1.53 | 0.00 | 1.00 | 16.83 | 14.98 | 37.09 | 296.95 | 0.6498 | -652.0 | -516.7 | |
| 0.00 | 1.28 | 0.00 | 0.80 | 14.74 | 13.17 | 35.28 | 294.82 | 0.6177 | -590.0 | -452.7 | |
| 0.00 | 1.02 | 0.00 | 0.64 | 14.98 | 12.65 | 34.76 | 295.48 | 0.6124 | -634.0 | -479.1 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 20.31 | 6.44 | 28.55 | 308.08 | 0.5717 | 705.0 | 549.4 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 19.64 | 3.98 | 26.09 | 309.42 | 0.5382 | 682.0 | 581.8 | |
| 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. | |