SDO HMI 2013-01-05 13:58:54 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.57 | 300.75 | 23.90 | 165.44 | -24.20 | 250.97 | -15.75 | 145.14 | 0.4346 | 778.7 | 344.8 | |
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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 |
| 42.47 | 285.99 | 23.29 | 157.02 | -24.17 | 251.30 | -15.42 | 145.58 | 0.4311 | 1426.3 | 399.0 | |
| 1.10 | -1.00 | 0.61 | -1.00 | -24.22 | 250.85 | -15.87 | 144.93 | 0.4357 | 932.6 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.86 | -26.53 | 248.40 | -18.32 | 144.42 | 0.4854 | 685.0 | 479.7 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -27.99 | 245.51 | -21.21 | 142.57 | 0.5277 | -708.0 | -526.9 | |
| 0.00 | 1.95 | 0.00 | 1.10 | -23.84 | 246.12 | -20.60 | 137.43 | 0.4778 | -868.0 | -691.4 | |
| 0.00 | 1.10 | 0.00 | 0.65 | -28.37 | 245.11 | -21.61 | 142.58 | 0.5354 | -677.0 | -472.8 | |
| 0.00 | 2.04 | 0.00 | 1.16 | -24.45 | 244.87 | -21.85 | 136.79 | 0.4970 | -920.0 | -789.5 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -24.28 | 244.41 | -22.31 | 135.98 | 0.5001 | -846.0 | -695.6 | |
| 0.00 | 0.76 | 0.00 | 0.43 | -23.39 | 244.33 | -22.39 | 134.51 | 0.4923 | -527.0 | -496.6 | |
| 0.00 | 1.78 | 0.00 | 1.02 | -23.96 | 244.19 | -22.53 | 135.23 | 0.4993 | -598.0 | -528.0 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -23.26 | 244.07 | -22.65 | 134.00 | 0.4938 | -869.0 | -720.9 | |
| 0.00 | 0.59 | 0.00 | 0.34 | -22.08 | 244.18 | -22.54 | 132.19 | 0.4815 | -614.0 | -573.1 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -23.32 | 243.82 | -22.90 | 133.80 | 0.4972 | -670.0 | -550.2 | |
| 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. | |