SDO HMI 2014-11-20 21:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.92 | 676.03 | 126.33 | 1037.56 | -13.41 | 164.45 | -69.33 | 105.07 | 0.9430 | 240.8 | -177.4 | |
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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 |
| 0.00 | 0.94 | 0.00 | 1.05 | -17.26 | 172.37 | -61.41 | 110.52 | 0.8972 | 506.0 | 449.4 | |
| 0.00 | 0.51 | 0.00 | 0.63 | -10.44 | 168.55 | -65.23 | 102.43 | 0.9161 | 366.0 | 295.7 | |
| 0.00 | 1.37 | 0.00 | 1.93 | -14.51 | 165.73 | -68.05 | 106.39 | 0.9375 | -290.0 | -286.4 | |
| 62.18 | 661.55 | 84.72 | 1011.55 | -13.02 | 166.23 | -67.55 | 104.88 | 0.9333 | 558.4 | -180.1 | |
| 1.46 | -4.00 | 2.50 | -4.00 | -14.20 | 161.67 | -72.11 | 105.53 | 0.9588 | -629.9 | 999999 | |
| 5.75 | -4.00 | 10.00 | -4.00 | -14.02 | 161.41 | -72.38 | 105.32 | 0.9600 | -630.6 | 999999 | |
| 9.09 | -4.00 | 16.94 | -4.00 | -14.65 | 160.35 | -73.43 | 105.84 | 0.9652 | -255.9 | 999999 | |
| 1.20 | 2.57 | 2.19 | 4.70 | -14.02 | 160.57 | -73.22 | 105.23 | 0.9639 | -422.1 | -363.2 | |
| 1.29 | -4.00 | 2.43 | -4.00 | -14.23 | 160.06 | -73.72 | 105.38 | 0.9662 | 34.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.69 | -11.31 | 162.13 | -71.65 | 102.58 | 0.9550 | -321.0 | -281.0 | |
| 0.00 | 3.00 | 0.00 | 5.63 | -13.79 | 160.11 | -73.68 | 104.94 | 0.9658 | -217.0 | -191.5 | |
| 2.92 | -4.00 | 5.40 | -4.00 | -13.45 | 160.29 | -73.50 | 104.60 | 0.9648 | -463.0 | 999999 | |
| 0.00 | 2.40 | 0.00 | 4.83 | -14.42 | 159.08 | -74.70 | 105.47 | 0.9704 | 269.0 | 233.6 | |
| 1.03 | 2.66 | 2.15 | 5.55 | -14.16 | 158.49 | -75.29 | 105.15 | 0.9727 | -94.8 | -47.9 | |
| 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. | |