SDO HMI 2014-12-08 04:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.24 | 0.00 | 7.48 | 15.99 | 15.56 | 9.68 | 329.23 | 0.3322 | -391.9 | -404.3 | |
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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 | 0.46 | 17.16 | 22.91 | 17.03 | 316.53 | 0.4085 | -759.0 | -642.2 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 8.94 | 21.42 | 15.54 | 300.43 | 0.3084 | -784.0 | -619.8 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 12.64 | 19.13 | 13.24 | 314.40 | 0.3143 | -721.0 | -579.8 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 16.51 | 17.86 | 11.97 | 325.03 | 0.3486 | -1000.0 | -787.4 | |
| 0.00 | 2.05 | 0.00 | 1.06 | 12.64 | 17.58 | 11.69 | 317.91 | 0.2964 | -838.0 | -723.0 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 13.70 | 17.60 | 11.72 | 320.22 | 0.3098 | -800.0 | -639.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 15.56 | 16.61 | 10.73 | 326.26 | 0.3243 | -830.0 | -681.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.66 | 14.86 | 8.98 | 336.42 | 0.3688 | -591.0 | -423.9 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 15.26 | 12.87 | 6.99 | 335.97 | 0.2897 | -675.0 | -591.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.91 | 9.69 | 3.81 | 349.62 | 0.3480 | 762.0 | 574.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.32 | 8.86 | 2.98 | 351.58 | 0.3361 | 817.0 | 692.2 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 21.09 | 3.48 | -2.40 | 6.20 | 0.3637 | 716.0 | 639.4 | |
| 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. | |