SDO HMI 2014-10-05 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.01 | 0.00 | 23.03 | 13.32 | 59.29 | -63.88 | 78.31 | 0.8938 | 15.5 | 134.7 | |
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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 | 1.84 | 0.00 | 1.83 | 14.42 | 62.47 | -60.70 | 77.07 | 0.8686 | -170.0 | -131.5 | |
| 0.00 | 1.23 | 0.00 | 1.22 | 14.02 | 62.46 | -60.71 | 77.53 | 0.8686 | -460.0 | -381.6 | |
| 0.00 | 0.44 | 0.00 | 0.47 | 13.09 | 59.90 | -63.27 | 78.59 | 0.8894 | -243.0 | -316.6 | |
| 0.00 | 1.23 | 0.00 | 1.33 | 13.41 | 59.68 | -63.49 | 78.23 | 0.8910 | -385.0 | -313.3 | |
| 0.00 | 1.76 | 0.00 | 1.91 | 13.04 | 59.65 | -63.52 | 78.65 | 0.8913 | -161.0 | -77.7 | |
| 0.00 | 0.97 | 0.00 | 1.04 | 12.86 | 59.73 | -63.44 | 78.85 | 0.8907 | -357.0 | -173.5 | |
| 0.00 | 1.41 | 0.00 | 1.55 | 13.87 | 59.10 | -64.07 | 77.70 | 0.8954 | -121.0 | -130.1 | |
| 0.00 | 0.97 | 0.00 | 1.06 | 13.52 | 59.27 | -63.89 | 78.10 | 0.8941 | -232.0 | -141.6 | |
| 0.00 | 1.41 | 0.00 | 1.54 | 13.17 | 59.38 | -63.79 | 78.50 | 0.8934 | 385.0 | 305.1 | |
| 0.00 | 3.25 | 0.00 | 3.62 | 13.45 | 58.88 | -64.29 | 78.17 | 0.8971 | 426.0 | 359.9 | |
| 0.00 | 0.88 | 0.00 | 1.00 | 14.23 | 58.33 | -64.83 | 77.30 | 0.9011 | -222.0 | -231.8 | |
| 0.00 | 2.90 | 0.00 | 3.30 | 12.83 | 58.17 | -65.00 | 78.86 | 0.9024 | 617.0 | 587.4 | |
| 0.00 | 1.14 | 0.00 | 1.31 | 12.37 | 57.88 | -65.29 | 79.36 | 0.9047 | 595.0 | 551.5 | |
| 0.00 | 1.58 | 0.00 | 1.85 | 12.72 | 57.41 | -65.76 | 78.96 | 0.9080 | 545.0 | 460.6 | |
| 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. | |