SDO HMI 2014-02-24 23:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.05 | 228.31 | 75.45 | 525.67 | -13.21 | 107.15 | -78.64 | 102.00 | 0.9764 | -108.8 | -293.8 | |
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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 | 0.69 | 0.00 | 0.60 | -11.87 | 129.51 | -56.28 | 99.51 | 0.8276 | 514.0 | 440.4 | |
| 0.00 | 0.86 | 0.00 | 0.84 | -15.02 | 125.40 | -60.39 | 103.24 | 0.8647 | 473.0 | 441.4 | |
| 0.00 | 0.95 | 0.00 | 0.94 | -15.66 | 124.83 | -60.96 | 103.98 | 0.8696 | 357.0 | 264.2 | |
| 0.00 | 0.60 | 0.00 | 0.58 | -11.09 | 125.84 | -59.96 | 98.68 | 0.8614 | 357.0 | 333.6 | |
| 0.00 | 1.12 | 0.00 | 1.72 | -16.20 | 113.30 | -72.49 | 104.73 | 0.9484 | 258.0 | 239.0 | |
| 0.00 | 3.01 | 0.00 | 4.67 | -16.00 | 113.18 | -72.62 | 104.53 | 0.9491 | 308.0 | 208.4 | |
| 0.00 | 2.24 | 0.00 | 4.00 | -11.71 | 110.87 | -74.93 | 100.17 | 0.9619 | 222.0 | 58.5 | |
| 9.04 | 208.26 | 20.23 | 485.01 | -14.29 | 107.18 | -78.62 | 103.10 | 0.9764 | -548.8 | -327.0 | |
| 0.00 | 5.85 | 0.00 | 14.91 | -15.23 | 105.47 | -80.32 | 104.18 | 0.9820 | 369.0 | 251.0 | |
| 0.00 | 4.73 | 0.00 | 12.40 | -14.65 | 105.28 | -80.52 | 103.61 | 0.9827 | -406.0 | -385.9 | |
| 24.01 | -8.00 | 55.22 | -8.00 | -12.64 | 106.97 | -78.82 | 101.43 | 0.9776 | -9.8 | 999999 | |
| 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. | |