SDO HMI 2014-11-11 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.83 | 0.00 | 8.06 | -10.82 | 338.15 | -19.79 | 125.97 | 0.4122 | -207.7 | -187.0 | |
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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 | 1.38 | 0.00 | 0.73 | -9.80 | 342.99 | -14.95 | 131.42 | 0.3404 | 868.0 | 714.1 | |
| 0.00 | 1.81 | 0.00 | 0.94 | -6.50 | 342.84 | -15.09 | 122.95 | 0.3097 | 850.0 | 639.3 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -13.31 | 340.37 | -17.56 | 133.91 | 0.4093 | 929.0 | 732.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -11.10 | 339.96 | -17.98 | 129.01 | 0.3915 | 710.0 | 571.2 | |
| 0.00 | 1.64 | 0.00 | 0.90 | -12.32 | 336.97 | -20.97 | 127.17 | 0.4405 | -936.0 | -822.5 | |
| 0.00 | 1.90 | 0.00 | 1.05 | -12.26 | 336.58 | -21.35 | 126.58 | 0.4449 | -697.0 | -575.5 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -10.27 | 336.55 | -21.39 | 122.69 | 0.4282 | -829.0 | -709.8 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -12.18 | 336.30 | -21.64 | 126.06 | 0.4477 | -794.0 | -569.2 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -10.15 | 336.36 | -21.57 | 122.23 | 0.4297 | -972.0 | -744.1 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -10.47 | 336.01 | -21.92 | 122.45 | 0.4369 | -604.0 | -525.0 | |
| 0.00 | 1.90 | 0.00 | 1.06 | -10.90 | 334.57 | -23.37 | 121.66 | 0.4594 | -810.0 | -637.3 | |
| 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. | |