SDO HMI 2014-01-12 04:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.77 | 84.26 | 18.18 | 44.03 | -17.89 | 29.48 | -12.94 | 138.17 | 0.3205 | 90.7 | 213.1 | |
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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 | 0.94 | 0.00 | 0.48 | -16.98 | 30.83 | -11.59 | 139.08 | 0.2948 | 837.0 | 604.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -17.22 | 30.66 | -11.77 | 139.23 | 0.2996 | 921.0 | 774.0 | |
| 14.45 | 37.32 | 7.51 | 19.41 | -17.55 | 30.44 | -11.98 | 139.48 | 0.3059 | 1175.9 | 686.8 | |
| 0.00 | 2.21 | 0.00 | 1.15 | -18.16 | 30.24 | -12.18 | 140.34 | 0.3155 | 747.0 | 689.3 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -17.25 | 30.21 | -12.21 | 138.26 | 0.3047 | 579.0 | 542.1 | |
| 1.87 | -3.00 | 0.97 | -3.00 | -17.55 | 30.07 | -12.36 | 138.61 | 0.3100 | 879.4 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -17.81 | 29.73 | -12.69 | 138.46 | 0.3169 | 501.0 | 304.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -16.87 | 29.48 | -12.94 | 135.77 | 0.3086 | 923.0 | 753.8 | |
| 0.00 | 3.23 | 0.00 | 1.69 | -17.41 | 29.38 | -13.04 | 136.81 | 0.3161 | 250.0 | 459.9 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -18.38 | 29.11 | -13.31 | 138.38 | 0.3304 | -677.0 | -495.7 | |
| 0.68 | 34.68 | 0.36 | 18.24 | -18.53 | 28.75 | -13.67 | 137.95 | 0.3361 | -961.5 | -603.3 | |
| 8.67 | -11.00 | 4.56 | -11.00 | -18.49 | 28.40 | -14.02 | 137.18 | 0.3396 | -1058.6 | 999999 | |
| 9.10 | -11.00 | 4.78 | -11.00 | -18.21 | 28.26 | -14.16 | 136.32 | 0.3379 | -1080.4 | 999999 | |
| 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. | |