SDO HMI 2014-11-22 12:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.24 | 0.00 | 9.07 | -12.96 | 225.75 | 13.37 | 220.97 | 0.3439 | 400.4 | 181.5 | |
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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 | 1.80 | 0.00 | 0.96 | -13.49 | 227.80 | 15.42 | 224.25 | 0.3721 | 943.0 | 823.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -12.33 | 227.73 | 15.35 | 226.45 | 0.3583 | 881.0 | 712.4 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -13.25 | 227.59 | 15.21 | 224.35 | 0.3670 | 946.0 | 786.5 | |
| 0.00 | 2.23 | 0.00 | 1.19 | -13.65 | 227.56 | 15.18 | 223.51 | 0.3711 | 801.0 | 759.1 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -12.14 | 227.37 | 14.99 | 226.18 | 0.3520 | 755.0 | 648.1 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -13.15 | 226.99 | 14.61 | 223.40 | 0.3590 | 1005.0 | 786.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -12.57 | 226.93 | 14.54 | 224.45 | 0.3516 | 923.0 | 766.0 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -12.84 | 226.91 | 14.53 | 223.86 | 0.3545 | 962.0 | 783.1 | |
| 0.00 | 2.66 | 0.00 | 1.39 | -13.98 | 223.35 | 10.97 | 213.96 | 0.3319 | -943.0 | -732.9 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -12.07 | 222.90 | 10.51 | 216.40 | 0.3020 | -926.0 | -732.2 | |
| 0.00 | 2.57 | 0.00 | 1.33 | -12.04 | 222.68 | 10.30 | 215.90 | 0.2995 | -943.0 | -833.2 | |
| 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. | |