SDO HMI 2011-01-07 16:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.64 | 0.00 | 15.99 | -14.05 | 206.52 | 39.49 | 252.58 | 0.6485 | -380.6 | -408.8 | |
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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 | 1.53 | 0.00 | 1.07 | -13.97 | 211.66 | 44.63 | 253.96 | 0.7117 | 659.0 | 484.7 | |
| 0.00 | 1.02 | 0.00 | 0.71 | -15.65 | 210.60 | 43.57 | 251.36 | 0.7028 | 515.0 | 432.6 | |
| 0.00 | 1.87 | 0.00 | 1.28 | -16.68 | 209.36 | 42.33 | 249.57 | 0.6908 | 611.0 | 470.5 | |
| 0.00 | 0.85 | 0.00 | 0.55 | -13.94 | 206.87 | 39.84 | 252.85 | 0.6531 | -457.0 | -408.3 | |
| 0.00 | 1.44 | 0.00 | 0.94 | -14.06 | 206.74 | 39.71 | 252.63 | 0.6517 | -645.0 | -523.0 | |
| 0.00 | 1.70 | 0.00 | 1.10 | -13.89 | 206.62 | 39.60 | 252.86 | 0.6498 | -591.0 | -527.2 | |
| 0.00 | 1.36 | 0.00 | 0.88 | -13.68 | 206.58 | 39.55 | 253.17 | 0.6488 | -606.0 | -567.9 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -13.70 | 205.96 | 38.93 | 252.95 | 0.6409 | -739.0 | -583.9 | |
| 0.00 | 1.02 | 0.00 | 0.65 | -13.92 | 205.73 | 38.70 | 252.55 | 0.6385 | -654.0 | -574.9 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -13.60 | 205.39 | 38.37 | 252.94 | 0.6333 | -649.0 | -604.9 | |
| 0.00 | 2.80 | 0.00 | 1.79 | -13.85 | 205.36 | 38.33 | 252.55 | 0.6336 | -670.0 | -679.5 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -13.62 | 205.13 | 38.10 | 252.84 | 0.6299 | -510.0 | -539.1 | |
| 0.00 | 5.27 | 0.00 | 3.34 | -13.42 | 204.86 | 37.83 | 253.07 | 0.6259 | -706.0 | -660.4 | |
| 0.00 | 1.70 | 0.00 | 1.08 | -13.87 | 204.86 | 37.84 | 252.37 | 0.6272 | -887.0 | -807.9 | |
| 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. | |