SDO HMI 2014-01-12 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.14 | 0.00 | 11.88 | 16.35 | 25.77 | -8.98 | 22.82 | 0.3855 | 40.2 | 60.9 | |
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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 | 1.27 | 0.00 | 0.68 | 16.50 | 30.28 | -4.47 | 11.91 | 0.3642 | -717.0 | -520.2 | |
| 0.00 | 2.12 | 0.00 | 1.12 | 15.56 | 29.25 | -5.50 | 15.22 | 0.3533 | -894.0 | -716.0 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.39 | 28.21 | -6.54 | 17.21 | 0.3710 | -847.0 | -735.4 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.33 | 27.94 | -6.82 | 17.94 | 0.3714 | -850.0 | -765.4 | |
| 0.00 | 2.29 | 0.00 | 1.22 | 16.28 | 27.32 | -7.43 | 19.50 | 0.3737 | -1126.0 | -925.4 | |
| 0.00 | 1.95 | 0.00 | 1.04 | 16.28 | 27.10 | -7.65 | 20.02 | 0.3750 | -856.0 | -659.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 16.93 | 25.24 | -9.51 | 23.65 | 0.3959 | 715.0 | 586.4 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 17.33 | 24.12 | -10.63 | 25.62 | 0.4091 | 755.0 | 560.1 | |
| 0.00 | 2.72 | 0.00 | 1.46 | 16.29 | 23.99 | -10.76 | 27.10 | 0.3952 | 956.0 | 772.2 | |
| 0.00 | 2.12 | 0.00 | 1.14 | 15.85 | 23.76 | -10.99 | 28.12 | 0.3907 | 953.0 | 886.6 | |
| 0.00 | 2.04 | 0.00 | 1.10 | 15.92 | 23.45 | -11.30 | 28.71 | 0.3941 | 857.0 | 697.6 | |
| 0.00 | 0.25 | 0.00 | 0.14 | 16.78 | 23.02 | -11.73 | 28.53 | 0.4093 | 698.0 | 602.7 | |
| 0.00 | 2.21 | 0.00 | 1.20 | 17.04 | 22.63 | -12.13 | 29.01 | 0.4159 | 878.0 | 710.4 | |
| 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. | |