SDO HMI 2014-01-10 12:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.18 | 0.00 | 12.80 | -17.19 | 69.85 | 5.46 | 207.82 | 0.3335 | -423.5 | -351.5 | |
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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 | 1.44 | 0.00 | 0.76 | -13.25 | 81.35 | 16.96 | 240.19 | 0.3286 | -674.0 | -531.2 | |
| 0.00 | 3.14 | 0.00 | 1.65 | -12.78 | 81.22 | 16.83 | 241.33 | 0.3232 | -774.0 | -674.6 | |
| 0.00 | 2.97 | 0.00 | 1.56 | -13.05 | 81.05 | 16.66 | 240.34 | 0.3228 | -765.0 | -745.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -12.64 | 80.71 | 16.32 | 241.02 | 0.3148 | -964.0 | -810.1 | |
| 0.00 | 2.12 | 0.00 | 1.10 | -16.72 | 76.57 | 12.18 | 222.48 | 0.3005 | 717.0 | 593.2 | |
| 0.00 | 2.04 | 0.00 | 1.05 | -15.50 | 75.96 | 11.57 | 224.09 | 0.2791 | 1015.0 | 751.0 | |
| 0.00 | 1.78 | 0.00 | 0.93 | -19.61 | 74.48 | 10.08 | 211.52 | 0.3169 | 933.0 | 578.2 | |
| 0.00 | 2.21 | 0.00 | 1.12 | -13.94 | 72.89 | 8.50 | 219.79 | 0.2251 | -720.0 | -556.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -11.24 | 71.41 | 7.02 | 223.70 | 0.1742 | -883.0 | -740.1 | |
| 0.00 | 1.78 | 0.00 | 0.92 | -15.82 | 54.50 | -9.89 | 141.09 | 0.2643 | -1046.0 | -808.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -25.10 | 52.87 | -11.52 | 153.33 | 0.4048 | -636.0 | -594.6 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -30.36 | 45.86 | -18.53 | 148.42 | 0.5258 | -667.0 | -637.3 | |
| 0.00 | 0.93 | 0.00 | 0.57 | -32.17 | 39.82 | -24.58 | 143.54 | 0.5947 | -759.0 | -594.5 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -26.93 | 40.42 | -23.97 | 137.41 | 0.5373 | -706.0 | -537.1 | |
| 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. | |