SDO HMI 2014-12-07 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.55 | 0.00 | 7.32 | -15.46 | 36.61 | 17.00 | 226.01 | 0.3920 | -239.9 | -184.3 | |
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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 | 0.77 | 0.00 | 0.43 | -19.26 | 41.27 | 21.66 | 226.41 | 0.4832 | 706.0 | 585.2 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -19.42 | 41.23 | 21.62 | 226.10 | 0.4842 | 668.0 | 575.3 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -15.17 | 39.44 | 19.83 | 231.15 | 0.4222 | 811.0 | 458.8 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -15.69 | 38.74 | 19.13 | 229.19 | 0.4187 | 849.0 | 654.7 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -12.67 | 37.01 | 17.41 | 232.82 | 0.3679 | -793.0 | -653.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -12.79 | 36.64 | 17.03 | 231.97 | 0.3642 | -774.0 | -714.2 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -13.00 | 36.15 | 16.54 | 230.71 | 0.3600 | -965.0 | -772.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -15.31 | 35.36 | 15.76 | 224.54 | 0.3751 | -762.0 | -563.9 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -15.13 | 35.29 | 15.68 | 224.76 | 0.3721 | -768.0 | -624.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | -15.53 | 35.16 | 15.55 | 223.76 | 0.3751 | -822.0 | -581.9 | |
| 0.00 | 2.05 | 0.00 | 1.07 | -15.43 | 30.52 | 10.91 | 214.25 | 0.3258 | -789.0 | -642.1 | |
| 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. | |