SDO HMI 2014-01-13 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.20 | 285.45 | 25.10 | 151.86 | 5.79 | 46.06 | 18.45 | 299.01 | 0.3599 | -1055.3 | -452.8 | |
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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 |
| 0.00 | 0.85 | 0.00 | 0.70 | 12.34 | 78.51 | 50.89 | 288.94 | 0.8037 | -465.0 | -434.9 | |
| 0.00 | 1.45 | 0.00 | 0.98 | 9.63 | 68.58 | 40.96 | 289.08 | 0.6862 | -464.0 | -411.3 | |
| 0.00 | 1.36 | 0.00 | 0.91 | 8.96 | 67.97 | 40.35 | 288.40 | 0.6764 | -779.0 | -614.9 | |
| 0.00 | 1.53 | 0.00 | 0.94 | 11.67 | 59.93 | 32.32 | 296.83 | 0.5890 | -726.0 | -648.7 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 4.92 | 53.82 | 26.20 | 289.26 | 0.4679 | -631.0 | -514.5 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 6.74 | 52.92 | 25.30 | 293.62 | 0.4652 | -813.0 | -674.5 | |
| 1.45 | 8.33 | 0.82 | 4.70 | 10.30 | 52.52 | 24.90 | 300.74 | 0.4839 | -752.1 | -724.7 | |
| 3.49 | -7.00 | 1.97 | -7.00 | 10.14 | 52.37 | 24.75 | 300.60 | 0.4808 | -991.2 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 9.89 | 47.78 | 20.16 | 305.45 | 0.4186 | -745.0 | -566.6 | |
| 42.26 | 263.08 | 22.31 | 138.94 | 5.49 | 45.36 | 17.75 | 298.93 | 0.3482 | -1387.8 | -454.7 | |
| 0.00 | 1.70 | 0.00 | 0.90 | 8.45 | 43.40 | 15.78 | 309.17 | 0.3485 | -837.0 | -709.5 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 7.88 | 41.83 | 14.21 | 310.80 | 0.3227 | -732.0 | -512.4 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 1.13 | 37.59 | 9.97 | 298.69 | 0.1982 | 783.0 | 609.8 | |
| 0.00 | 1.53 | 0.00 | 0.78 | 7.17 | 36.38 | 8.76 | 322.82 | 0.2512 | 846.0 | 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. | |