SDO HMI 2014-11-22 05:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.00 | 0.00 | 10.41 | -13.52 | 225.33 | 9.13 | 209.89 | 0.3121 | -357.2 | -47.4 | |
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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 | 2.66 | 0.00 | 1.39 | -13.42 | 227.65 | 11.45 | 216.04 | 0.3296 | 921.0 | 755.4 | |
| 0.00 | 2.66 | 0.00 | 1.39 | -13.61 | 227.50 | 11.30 | 215.36 | 0.3306 | 689.0 | 613.7 | |
| 0.00 | 2.57 | 0.00 | 1.34 | -12.04 | 227.31 | 11.11 | 217.89 | 0.3081 | 381.0 | 443.3 | |
| 0.00 | 1.46 | 0.00 | 0.79 | -19.42 | 227.69 | 11.49 | 207.25 | 0.4119 | -749.0 | -577.5 | |
| 0.00 | 1.89 | 0.00 | 0.98 | -11.73 | 226.59 | 10.39 | 216.69 | 0.2968 | 809.0 | 672.5 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -10.22 | 223.52 | 7.32 | 210.66 | 0.2470 | -748.0 | -538.6 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -12.05 | 223.32 | 7.12 | 206.56 | 0.2723 | -816.0 | -626.4 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -14.19 | 223.35 | 7.15 | 203.41 | 0.3051 | -818.0 | -723.8 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -13.98 | 223.22 | 7.02 | 203.33 | 0.3009 | -809.0 | -646.9 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -12.07 | 222.74 | 6.54 | 204.63 | 0.2685 | -931.0 | -777.9 | |
| 0.00 | 1.97 | 0.00 | 1.01 | -11.98 | 222.53 | 6.33 | 204.06 | 0.2656 | -1043.0 | -850.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -13.76 | 222.42 | 6.22 | 201.18 | 0.2924 | -744.0 | -601.3 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -16.85 | 220.95 | 4.75 | 193.79 | 0.3342 | -786.0 | -664.1 | |
| 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. | |