SDO HMI 2014-11-28 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.13 | 37.04 | 4.39 | 20.00 | 17.31 | 151.79 | 17.39 | 314.28 | 0.4001 | 153.0 | -106.3 | |
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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 | 1.63 | 0.00 | 0.89 | 18.05 | 153.59 | 19.20 | 312.91 | 0.4286 | 866.0 | 748.8 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 17.01 | 153.21 | 18.82 | 311.52 | 0.4137 | 721.0 | 585.5 | |
| 4.11 | 12.06 | 2.24 | 6.58 | 17.93 | 153.08 | 18.69 | 313.42 | 0.4216 | 987.0 | 614.9 | |
| 0.68 | -3.00 | 0.37 | -3.00 | 18.12 | 153.01 | 18.61 | 313.88 | 0.4226 | 762.6 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 18.09 | 152.61 | 18.21 | 314.42 | 0.4178 | 843.0 | 775.4 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 16.41 | 151.50 | 17.10 | 312.97 | 0.3872 | 284.0 | 411.4 | |
| 0.00 | 2.57 | 0.00 | 1.38 | 16.65 | 150.94 | 16.54 | 314.37 | 0.3833 | -654.0 | -525.3 | |
| 2.14 | 11.29 | 1.14 | 6.04 | 16.35 | 150.75 | 16.36 | 314.08 | 0.3778 | -1043.2 | -837.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.35 | 150.84 | 16.45 | 317.70 | 0.4010 | -735.0 | -514.0 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 18.41 | 150.65 | 16.26 | 318.13 | 0.3997 | -825.0 | -653.6 | |
| 1.20 | 2.99 | 0.64 | 1.60 | 17.43 | 149.91 | 15.52 | 317.63 | 0.3804 | -1049.1 | -841.0 | |
| 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. | |