SDO HMI 2014-03-16 05:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.91 | 91.84 | 26.74 | 257.03 | 5.86 | 11.01 | 78.83 | 277.32 | 0.9846 | 230.4 | 60.0 | |
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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 | 1.48 | 0.00 | 4.66 | 3.01 | 12.72 | 80.54 | 274.22 | 0.9884 | 259.0 | 225.1 | |
| 0.00 | 0.78 | 0.00 | 3.10 | 6.35 | 13.97 | 81.79 | 277.38 | 0.9925 | -177.0 | -33.0 | |
| 0.00 | 6.26 | 0.00 | 24.22 | 6.70 | 13.82 | 81.65 | 277.75 | 0.9923 | -133.0 | -93.6 | |
| 0.00 | 1.04 | 0.00 | 3.22 | 5.06 | 12.15 | 79.97 | 276.35 | 0.9877 | -250.0 | -286.1 | |
| 0.52 | 7.83 | 1.53 | 22.47 | 5.30 | 11.58 | 79.41 | 276.67 | 0.9862 | -157.2 | -276.3 | |
| 0.00 | 3.04 | 0.00 | 7.58 | 3.69 | 10.14 | 77.97 | 275.26 | 0.9810 | -265.0 | -212.3 | |
| 5.22 | 66.01 | 14.25 | 178.90 | 5.86 | 10.75 | 78.58 | 277.36 | 0.9840 | 195.1 | 129.1 | |
| 0.00 | 0.78 | 0.00 | 1.89 | 4.06 | 9.68 | 77.51 | 275.70 | 0.9796 | 193.0 | 137.9 | |
| 4.17 | -7.00 | 10.96 | -7.00 | 6.30 | 10.38 | 78.20 | 277.86 | 0.9830 | 445.6 | 999999 | |
| 0.00 | 2.09 | 0.00 | 4.98 | 4.37 | 9.51 | 77.34 | 276.04 | 0.9792 | 360.0 | 295.4 | |
| 0.00 | 1.57 | 0.00 | 3.77 | 4.93 | 9.58 | 77.41 | 276.59 | 0.9797 | 427.0 | 375.2 | |
| 0.00 | 0.96 | 0.00 | 2.24 | 7.12 | 8.85 | 76.67 | 278.92 | 0.9783 | 398.0 | 216.2 | |
| 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. | |