SDO HMI 2014-05-23 02:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.21 | 50.88 | 8.23 | 27.41 | -13.66 | 135.68 | 19.90 | 237.73 | 0.3925 | 194.0 | -48.6 | |
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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 |
| 4.05 | 9.28 | 2.21 | 5.05 | -13.51 | 137.46 | 21.67 | 240.19 | 0.4156 | 916.6 | 708.8 | |
| 1.80 | -1.00 | 0.98 | -1.00 | -13.29 | 137.41 | 21.62 | 240.60 | 0.4133 | 1029.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -13.11 | 137.19 | 21.40 | 240.77 | 0.4090 | 837.0 | 713.2 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -13.70 | 136.98 | 21.19 | 239.25 | 0.4103 | 716.0 | 597.2 | |
| 4.41 | 6.76 | 2.39 | 3.66 | -13.11 | 136.79 | 21.00 | 240.33 | 0.4034 | 1058.2 | 835.7 | |
| 1.44 | 5.22 | 0.78 | 2.83 | -13.98 | 136.73 | 20.95 | 238.37 | 0.4092 | 939.6 | 822.8 | |
| 0.00 | 4.05 | 0.00 | 2.20 | -14.39 | 136.54 | 20.75 | 237.27 | 0.4097 | 841.0 | 715.2 | |
| 0.00 | 1.62 | 0.00 | 0.87 | -14.09 | 135.54 | 19.76 | 236.71 | 0.3939 | -679.0 | -492.3 | |
| 0.90 | 3.78 | 0.48 | 2.02 | -13.75 | 134.55 | 18.77 | 236.17 | 0.3778 | -817.1 | -541.8 | |
| 0.00 | 0.63 | 0.00 | 0.34 | -14.04 | 134.38 | 18.59 | 235.30 | 0.3778 | -535.0 | -494.3 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -14.13 | 133.96 | 18.17 | 234.49 | 0.3731 | -836.0 | -663.2 | |
| 0.00 | 2.16 | 0.00 | 1.16 | -14.72 | 134.01 | 18.22 | 233.25 | 0.3790 | -774.0 | -552.2 | |
| 2.61 | 13.60 | 1.39 | 7.24 | -13.45 | 133.80 | 18.02 | 235.84 | 0.3651 | -1085.5 | -831.9 | |
| 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. | |