SDO HMI 2014-12-06 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.81 | 0.00 | 11.02 | 13.43 | 16.48 | -15.21 | 48.17 | 0.3444 | -584.5 | -503.6 | |
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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 | 1.37 | 0.00 | 0.71 | 14.70 | 22.10 | -9.59 | 32.83 | 0.2987 | -842.0 | -639.0 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 9.03 | 21.05 | -10.65 | 50.02 | 0.2392 | -747.0 | -630.6 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.56 | 20.10 | -11.59 | 32.75 | 0.3557 | -804.0 | -640.4 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 13.79 | 18.50 | -13.19 | 43.37 | 0.3240 | -784.0 | -564.1 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 12.88 | 17.93 | -13.76 | 46.63 | 0.3204 | -850.0 | -585.8 | |
| 0.00 | 4.52 | 0.00 | 2.34 | 9.96 | 17.86 | -13.84 | 54.34 | 0.2912 | -862.0 | -819.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 9.21 | 17.79 | -13.90 | 56.63 | 0.2852 | -914.0 | -737.6 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 9.93 | 17.55 | -14.14 | 55.00 | 0.2952 | -755.0 | -630.1 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 9.72 | 17.43 | -14.26 | 55.81 | 0.2948 | -836.0 | -688.2 | |
| 0.00 | 2.30 | 0.00 | 1.21 | 13.37 | 16.93 | -14.76 | 47.48 | 0.3378 | -885.0 | -813.5 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 16.24 | 13.52 | -18.17 | 47.34 | 0.4089 | -773.0 | -607.8 | |
| 0.00 | 1.79 | 0.00 | 1.01 | 18.19 | 9.27 | -22.42 | 49.59 | 0.4778 | 818.0 | 642.4 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 21.93 | 4.51 | -27.18 | 48.87 | 0.5647 | 636.0 | 541.8 | |
| 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. | |