SDO HMI 2014-12-07 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.58 | 0.00 | 9.55 | 13.87 | 16.98 | 0.65 | 348.32 | 0.2528 | -627.9 | -614.0 | |
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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 | 1.19 | 0.00 | 0.63 | 17.02 | 26.37 | 10.04 | 330.22 | 0.3370 | -714.0 | -595.0 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 14.81 | 23.97 | 7.64 | 333.18 | 0.2860 | -722.0 | -619.3 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 12.62 | 21.31 | 4.97 | 338.71 | 0.2340 | -891.0 | -720.4 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 17.58 | 18.48 | 2.15 | 353.22 | 0.3041 | -723.0 | -575.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 12.39 | 17.49 | 1.15 | 354.73 | 0.2149 | -880.0 | -745.1 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 12.63 | 17.49 | 1.15 | 354.82 | 0.2190 | -838.0 | -654.7 | |
| 0.00 | 1.28 | 0.00 | 0.65 | 12.17 | 17.30 | 0.97 | 355.48 | 0.2110 | -1066.0 | -832.1 | |
| 0.00 | 2.64 | 0.00 | 1.33 | 9.98 | 17.14 | 0.81 | 355.36 | 0.1732 | -950.0 | -765.9 | |
| 0.00 | 2.13 | 0.00 | 1.08 | 13.14 | 17.16 | 0.82 | 356.45 | 0.2274 | -938.0 | -749.3 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 11.69 | 16.67 | 0.34 | 358.37 | 0.2022 | -745.0 | -620.4 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 14.91 | 13.19 | -3.14 | 11.69 | 0.2625 | -863.0 | -733.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 15.74 | 13.09 | -3.24 | 11.42 | 0.2765 | -738.0 | -608.2 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 24.44 | 359.02 | -17.31 | 33.29 | 0.4955 | 786.0 | 667.1 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 19.39 | 354.12 | -22.21 | 47.16 | 0.4883 | 491.0 | 543.5 | |
| 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. | |