SDO HMI 2014-12-08 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.07 | 0.00 | 7.50 | 14.66 | 15.83 | 13.76 | 320.20 | 0.3674 | -400.2 | -371.6 | |
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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 | 1.11 | 0.00 | 0.63 | 13.77 | 28.43 | 26.36 | 298.98 | 0.4950 | -741.0 | -572.2 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 13.53 | 23.18 | 21.12 | 303.83 | 0.4235 | -685.0 | -631.6 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 12.71 | 22.43 | 20.36 | 303.05 | 0.4067 | -804.0 | -683.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 10.33 | 20.81 | 18.75 | 299.67 | 0.3655 | -774.0 | -675.3 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 14.29 | 19.57 | 17.51 | 310.35 | 0.3842 | -770.0 | -599.2 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 16.47 | 17.90 | 15.83 | 317.38 | 0.3881 | -900.0 | -772.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 13.63 | 17.36 | 15.30 | 312.67 | 0.3503 | -825.0 | -583.3 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 12.05 | 16.92 | 14.85 | 309.89 | 0.3282 | -750.0 | -685.8 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 12.54 | 15.64 | 13.57 | 313.56 | 0.3175 | -854.0 | -697.2 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 19.65 | 8.88 | 6.81 | 341.66 | 0.3567 | 683.0 | 540.2 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 20.00 | 4.58 | 2.51 | 353.15 | 0.3468 | 793.0 | 618.0 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 17.88 | 359.61 | -2.46 | 7.55 | 0.3119 | 824.0 | 607.1 | |
| 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. | |