SDO HMI 2014-12-07 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.30 | 0.00 | 8.65 | 16.11 | 12.14 | -9.12 | 318.43 | 0.3337 | -94.5 | -97.8 | |
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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 | 1.54 | 0.00 | 0.79 | 15.42 | 25.16 | 3.91 | 346.00 | 0.2727 | -804.0 | -620.7 | |
| 0.00 | 2.73 | 0.00 | 1.39 | 13.87 | 22.85 | 1.59 | 353.51 | 0.2398 | -730.0 | -547.6 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.23 | 18.17 | -3.08 | 16.84 | 0.1836 | -989.0 | -785.6 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 9.87 | 17.75 | -3.50 | 19.63 | 0.1800 | -932.0 | -747.4 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 12.30 | 17.00 | -4.25 | 19.00 | 0.2237 | -866.0 | -654.4 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.42 | 15.67 | -5.58 | 22.40 | 0.2495 | -899.0 | -760.2 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 19.69 | 8.88 | -12.37 | 31.10 | 0.3922 | 596.0 | 517.1 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 19.56 | 4.78 | -16.47 | 38.79 | 0.4283 | 858.0 | 590.7 | |
| 0.00 | 1.71 | 0.00 | 0.94 | 19.72 | 4.34 | -16.92 | 39.27 | 0.4346 | 835.0 | 553.3 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 24.09 | 359.26 | -22.00 | 40.11 | 0.5328 | 680.0 | 591.5 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 17.42 | 357.70 | -23.55 | 52.07 | 0.4853 | 508.0 | 483.3 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 19.85 | 355.27 | -25.99 | 50.70 | 0.5347 | 609.0 | 468.1 | |
| 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. | |