SDO HMI 2014-01-08 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.84 | 0.00 | 8.50 | -18.56 | 67.24 | -24.59 | 126.11 | 0.4754 | -116.5 | -42.0 | |
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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 | 1.87 | 0.00 | 0.97 | -19.27 | 83.60 | -8.22 | 153.13 | 0.3001 | 869.0 | 709.0 | |
| 0.00 | 1.70 | 0.00 | 0.90 | -16.55 | 75.13 | -16.70 | 128.95 | 0.3557 | 864.0 | 617.2 | |
| 0.00 | 1.95 | 0.00 | 1.06 | -20.21 | 73.47 | -18.36 | 133.94 | 0.4123 | 796.0 | 638.4 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -20.45 | 73.24 | -18.59 | 134.06 | 0.4174 | 849.0 | 650.1 | |
| 0.00 | 1.61 | 0.00 | 0.85 | -13.67 | 73.81 | -18.02 | 120.03 | 0.3487 | -787.0 | -576.5 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -12.65 | 68.78 | -23.04 | 112.50 | 0.4151 | -772.0 | -697.9 | |
| 0.00 | 1.10 | 0.00 | 0.66 | -14.91 | 58.83 | -32.99 | 111.03 | 0.5660 | -673.0 | -584.6 | |
| 0.00 | 0.93 | 0.00 | 0.57 | -15.79 | 57.90 | -33.93 | 112.07 | 0.5818 | -531.0 | -425.8 | |
| 0.00 | 0.76 | 0.00 | 0.51 | -24.84 | 54.37 | -37.45 | 123.90 | 0.6672 | -495.0 | -446.4 | |
| 0.00 | 0.68 | 0.00 | 0.46 | -23.60 | 52.59 | -39.24 | 121.25 | 0.6804 | -755.0 | -665.6 | |
| 0.00 | 1.61 | 0.00 | 1.09 | -23.21 | 52.31 | -39.52 | 120.58 | 0.6816 | -647.0 | -515.0 | |
| 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. | |