SDO HMI 2014-11-23 15:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.75 | 0.00 | 10.91 | -12.46 | 225.74 | 28.18 | 242.08 | 0.5232 | -93.1 | 8.6 | |
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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 | 1.88 | 0.00 | 1.13 | -13.41 | 228.78 | 31.23 | 242.86 | 0.5689 | 537.0 | 483.5 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -12.40 | 228.50 | 30.95 | 244.32 | 0.5595 | 725.0 | 649.7 | |
| 0.00 | 0.43 | 0.00 | 0.26 | -13.10 | 228.53 | 30.97 | 243.18 | 0.5638 | 626.0 | 598.6 | |
| 0.00 | 3.68 | 0.00 | 2.20 | -12.76 | 228.27 | 30.71 | 243.56 | 0.5585 | 738.0 | 656.6 | |
| 0.00 | 1.63 | 0.00 | 0.97 | -12.82 | 227.92 | 30.37 | 243.23 | 0.5543 | 832.0 | 745.6 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -11.89 | 223.91 | 26.36 | 241.68 | 0.4956 | -655.0 | -540.2 | |
| 0.00 | 2.31 | 0.00 | 1.31 | -11.55 | 223.51 | 25.95 | 241.96 | 0.4878 | -817.0 | -665.1 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -12.44 | 223.50 | 25.94 | 240.33 | 0.4937 | -797.0 | -611.7 | |
| 0.00 | 2.74 | 0.00 | 1.55 | -12.10 | 223.29 | 25.74 | 240.76 | 0.4887 | -562.0 | -272.0 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -12.46 | 223.30 | 25.74 | 240.10 | 0.4913 | -841.0 | -664.0 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -12.65 | 223.25 | 25.70 | 239.72 | 0.4919 | -810.0 | -655.2 | |
| 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. | |