SDO HMI 2014-11-22 02:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.58 | 0.00 | 12.29 | -13.92 | 225.67 | 7.83 | 205.09 | 0.3093 | -412.5 | -354.5 | |
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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 | 4.03 | 0.00 | 2.15 | -15.27 | 231.33 | 13.49 | 217.21 | 0.3737 | -775.0 | -600.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -12.90 | 228.68 | 10.83 | 215.48 | 0.3170 | 872.0 | 704.6 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -19.28 | 227.53 | 9.68 | 203.63 | 0.3979 | -912.0 | -664.6 | |
| 0.00 | 1.72 | 0.00 | 0.89 | -13.13 | 227.14 | 9.30 | 211.07 | 0.3062 | 853.0 | 656.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -12.30 | 226.84 | 8.99 | 211.71 | 0.2918 | 887.0 | 710.9 | |
| 0.00 | 1.97 | 0.00 | 1.03 | -13.28 | 226.78 | 8.93 | 209.82 | 0.3053 | 801.0 | 656.5 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -11.92 | 223.47 | 5.62 | 201.70 | 0.2604 | -796.0 | -606.1 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -12.38 | 223.35 | 5.51 | 200.67 | 0.2669 | -933.0 | -737.5 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -10.67 | 223.32 | 5.48 | 203.13 | 0.2400 | -981.0 | -767.4 | |
| 0.00 | 1.80 | 0.00 | 0.92 | -12.13 | 223.32 | 5.47 | 200.88 | 0.2628 | -1054.0 | -916.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -13.94 | 223.20 | 5.36 | 198.25 | 0.2908 | -753.0 | -591.9 | |
| 0.00 | 2.83 | 0.00 | 1.46 | -13.63 | 223.14 | 5.29 | 198.38 | 0.2856 | -925.0 | -704.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -11.94 | 222.40 | 4.56 | 197.86 | 0.2547 | -836.0 | -708.6 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -17.01 | 221.01 | 3.17 | 189.21 | 0.3318 | -890.0 | -743.6 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -17.29 | 220.96 | 3.11 | 188.91 | 0.3363 | -746.0 | -602.5 | |
| 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. | |