SDO HMI 2014-09-03 19:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.78 | 0.00 | 11.41 | 9.65 | 181.43 | -2.50 | 225.52 | 0.1151 | -320.1 | -313.9 | |
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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 | 1.07 | 0.00 | 0.53 | 5.24 | 189.75 | 5.82 | 251.39 | 0.1071 | -886.0 | -679.1 | |
| 0.00 | 1.52 | 0.00 | 0.75 | 6.08 | 187.26 | 3.33 | 251.16 | 0.0614 | -1157.0 | -926.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 11.56 | 186.36 | 2.43 | 331.25 | 0.0868 | -787.0 | -610.0 | |
| 0.00 | 2.59 | 0.00 | 1.29 | 10.87 | 185.95 | 2.02 | 331.40 | 0.0728 | -811.0 | -756.4 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.38 | 185.93 | 2.00 | 334.79 | 0.0806 | -1018.0 | -740.4 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 11.96 | 185.75 | 1.82 | 339.42 | 0.0887 | -605.0 | -448.8 | |
| 0.00 | 3.04 | 0.00 | 1.51 | 5.97 | 185.31 | 1.39 | 227.81 | 0.0326 | -1004.0 | -827.9 | |
| 0.00 | 1.52 | 0.00 | 0.75 | 6.03 | 185.10 | 1.17 | 224.47 | 0.0292 | -892.0 | -586.5 | |
| 0.00 | 1.88 | 0.00 | 0.93 | 10.96 | 184.81 | 0.89 | 346.90 | 0.0673 | -823.0 | -657.0 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 11.33 | 184.82 | 0.89 | 348.02 | 0.0735 | -823.0 | -718.2 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 10.07 | 178.82 | -5.11 | 60.27 | 0.1014 | 929.0 | 702.7 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 9.66 | 172.47 | -11.46 | 77.08 | 0.2018 | 741.0 | 558.1 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 11.38 | 171.05 | -12.88 | 70.92 | 0.2322 | 781.0 | 641.4 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 12.84 | 163.99 | -19.93 | 72.43 | 0.3502 | 842.0 | 607.1 | |
| 0.00 | 0.71 | 0.00 | 0.38 | 16.16 | 162.40 | -21.52 | 65.07 | 0.3903 | 711.0 | 567.9 | |
| 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. | |