SDO HMI 2014-01-02 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.76 | 44.86 | 11.58 | 39.41 | -11.97 | 116.40 | -55.53 | 102.37 | 0.8258 | 367.5 | 213.3 | |
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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 |
| 8.24 | 24.99 | 6.77 | 20.46 | -11.38 | 119.16 | -52.77 | 101.88 | 0.7999 | 855.7 | 527.9 | |
| 0.00 | 1.36 | 0.00 | 1.14 | -13.67 | 118.48 | -53.46 | 104.64 | 0.8091 | 398.0 | 373.0 | |
| 5.52 | 8.33 | 4.81 | 7.26 | -12.38 | 116.75 | -55.18 | 102.87 | 0.8247 | 571.4 | 360.8 | |
| 0.00 | 0.85 | 0.00 | 0.81 | -13.52 | 113.22 | -58.72 | 103.89 | 0.8581 | 326.0 | 261.9 | |
| 0.00 | 0.42 | 0.00 | 0.40 | -12.47 | 113.50 | -58.43 | 102.69 | 0.8549 | 161.0 | 252.4 | |
| 0.00 | 1.36 | 0.00 | 1.30 | -12.40 | 113.23 | -58.70 | 102.59 | 0.8572 | 304.0 | 252.5 | |
| 0.00 | 0.68 | 0.00 | 0.68 | -13.57 | 111.69 | -60.24 | 103.81 | 0.8711 | -531.0 | -502.2 | |
| 0.00 | 0.59 | 0.00 | 0.60 | -13.89 | 111.43 | -60.51 | 104.16 | 0.8735 | -440.0 | -414.1 | |
| 0.00 | 2.29 | 0.00 | 2.29 | -12.64 | 111.83 | -60.11 | 102.76 | 0.8694 | -429.0 | -504.6 | |
| 0.00 | 1.70 | 0.00 | 1.74 | -11.60 | 110.86 | -61.07 | 101.51 | 0.8769 | -268.0 | -268.5 | |
| 0.00 | 2.29 | 0.00 | 2.73 | -12.77 | 106.49 | -65.44 | 102.60 | 0.9107 | -500.0 | -378.2 | |
| 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. | |