SDO HMI 2014-12-06 14:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.89 | 0.00 | 9.37 | -15.47 | 36.83 | 10.05 | 211.48 | 0.3197 | -461.1 | -416.3 | |
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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 | 1.45 | 0.00 | 0.80 | -20.87 | 43.48 | 16.70 | 216.77 | 0.4506 | -847.0 | -639.4 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -19.44 | 40.57 | 13.79 | 213.77 | 0.4061 | 916.0 | 672.6 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -15.23 | 38.99 | 12.22 | 217.52 | 0.3368 | 943.0 | 781.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -15.04 | 37.73 | 10.96 | 214.94 | 0.3221 | 837.0 | 638.3 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -12.97 | 36.99 | 10.21 | 217.19 | 0.2872 | -803.0 | -600.1 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -13.12 | 35.89 | 9.11 | 213.81 | 0.2785 | -816.0 | -661.0 | |
| 0.00 | 2.13 | 0.00 | 1.10 | -14.46 | 35.45 | 8.67 | 209.99 | 0.2934 | -1025.0 | -858.6 | |
| 0.00 | 2.47 | 0.00 | 1.28 | -14.52 | 35.23 | 8.46 | 209.27 | 0.2925 | -869.0 | -727.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.19 | 35.13 | 8.36 | 207.87 | 0.3015 | -787.0 | -636.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -15.56 | 35.12 | 8.34 | 207.24 | 0.3068 | -638.0 | -639.9 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -14.64 | 34.93 | 8.15 | 208.19 | 0.2918 | -937.0 | -744.5 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -14.82 | 34.87 | 8.10 | 207.72 | 0.2941 | -863.0 | -756.5 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -14.94 | 34.85 | 8.07 | 207.45 | 0.2957 | -800.0 | -671.9 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -12.51 | 34.31 | 7.53 | 210.19 | 0.2557 | -766.0 | -688.8 | |
| 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. | |