SDO HMI 2014-11-23 10:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.09 | 0.00 | 10.22 | -12.44 | 225.39 | 25.10 | 239.39 | 0.4826 | -71.9 | -108.7 | |
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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 | 0.86 | 0.00 | 0.50 | -12.34 | 228.56 | 28.26 | 242.43 | 0.5239 | 548.0 | 459.8 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -12.89 | 228.35 | 28.05 | 241.32 | 0.5246 | 736.0 | 574.6 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -12.70 | 228.15 | 27.86 | 241.48 | 0.5208 | 880.0 | 732.0 | |
| 0.00 | 2.57 | 0.00 | 1.49 | -12.91 | 227.87 | 27.57 | 240.89 | 0.5185 | 769.0 | 708.9 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -13.80 | 227.77 | 27.48 | 239.28 | 0.5233 | 541.0 | 522.9 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -11.94 | 223.96 | 23.67 | 239.03 | 0.4599 | -557.0 | -425.6 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -11.78 | 223.81 | 23.52 | 239.18 | 0.4568 | -611.0 | -510.8 | |
| 0.00 | 3.77 | 0.00 | 2.09 | -11.53 | 223.46 | 23.17 | 239.30 | 0.4502 | -795.0 | -701.6 | |
| 0.00 | 2.40 | 0.00 | 1.33 | -11.87 | 223.43 | 23.13 | 238.61 | 0.4523 | -908.0 | -778.1 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -13.24 | 223.26 | 22.96 | 235.82 | 0.4610 | -764.0 | -587.5 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -13.58 | 223.29 | 23.00 | 235.24 | 0.4642 | -630.0 | -489.5 | |
| 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. | |