SDO HMI 2014-11-20 07:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.30 | 422.16 | 111.48 | 1031.27 | -13.28 | 165.09 | -76.39 | 104.15 | 0.9756 | 126.0 | -189.4 | |
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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 |
| 42.23 | 407.22 | 85.80 | 978.29 | -12.98 | 166.56 | -74.92 | 103.98 | 0.9707 | 303.5 | -204.8 | |
| 0.00 | 0.52 | 0.00 | 0.91 | -10.44 | 168.43 | -73.04 | 101.55 | 0.9614 | 103.0 | 92.2 | |
| 0.00 | 1.37 | 0.00 | 3.04 | -11.14 | 165.13 | -76.34 | 101.97 | 0.9756 | -442.0 | -357.6 | |
| 2.58 | -1.00 | 8.92 | -1.00 | -14.71 | 160.64 | -80.84 | 105.22 | 0.9902 | -86.0 | 999999 | |
| 0.00 | 0.60 | 0.00 | 1.34 | -10.96 | 165.02 | -76.45 | 101.78 | 0.9760 | -421.0 | -371.4 | |
| 5.49 | -1.00 | 16.76 | -1.00 | -13.94 | 161.65 | -79.82 | 104.52 | 0.9875 | -533.5 | 999999 | |
| 0.00 | 2.15 | 0.00 | 9.11 | -14.96 | 159.09 | -82.38 | 105.36 | 0.9936 | 452.0 | 373.2 | |
| 0.00 | 2.40 | 0.00 | 8.53 | -13.96 | 160.28 | -81.19 | 104.43 | 0.9909 | 248.0 | 231.5 | |
| 0.00 | 2.15 | 0.00 | 9.23 | -14.42 | 158.75 | -82.73 | 104.79 | 0.9941 | -245.0 | -82.6 | |
| 0.00 | 0.26 | 0.00 | 0.90 | -13.40 | 160.36 | -81.11 | 103.88 | 0.9906 | -342.0 | -347.0 | |
| 0.00 | 1.20 | 0.00 | 4.27 | -13.31 | 160.30 | -81.17 | 103.79 | 0.9908 | -276.0 | -194.6 | |
| 0.00 | 0.43 | 0.00 | 1.48 | -13.13 | 160.39 | -81.08 | 103.60 | 0.9905 | -216.0 | -242.2 | |
| 0.00 | 3.86 | 0.00 | 14.17 | -12.80 | 160.07 | -81.41 | 103.25 | 0.9912 | 112.0 | 120.4 | |
| 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. | |