SDO HMI 2014-05-23 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.88 | 72.35 | 17.83 | 40.24 | -13.70 | 136.40 | 24.46 | 242.30 | 0.4559 | 229.9 | 25.6 | |
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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 |
| 10.90 | 16.22 | 6.13 | 9.11 | -13.39 | 137.85 | 25.90 | 244.21 | 0.4739 | 977.8 | 640.6 | |
| 1.17 | 7.57 | 0.66 | 4.23 | -12.96 | 137.45 | 25.51 | 244.75 | 0.4659 | 1062.7 | 906.6 | |
| 0.90 | -2.00 | 0.50 | -2.00 | -13.05 | 137.36 | 25.41 | 244.49 | 0.4651 | 1100.3 | 999999 | |
| 11.62 | 16.22 | 6.52 | 9.10 | -13.92 | 137.42 | 25.48 | 242.82 | 0.4712 | 1040.1 | 574.2 | |
| 1.26 | 6.40 | 0.71 | 3.59 | -14.36 | 137.13 | 25.18 | 241.72 | 0.4700 | 606.6 | 443.1 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -13.22 | 136.72 | 24.78 | 243.64 | 0.4572 | 883.0 | 730.0 | |
| 2.25 | 5.05 | 1.25 | 2.79 | -14.00 | 135.51 | 23.56 | 240.96 | 0.4454 | -824.5 | -689.7 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -13.54 | 135.39 | 23.44 | 241.80 | 0.4407 | -648.0 | -615.1 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -14.10 | 134.97 | 23.02 | 240.24 | 0.4388 | -602.0 | -411.2 | |
| 0.00 | 0.63 | 0.00 | 0.34 | -13.15 | 134.27 | 22.32 | 241.54 | 0.4224 | -617.0 | -645.7 | |
| 0.00 | 2.34 | 0.00 | 1.28 | -13.92 | 134.14 | 22.19 | 239.76 | 0.4261 | -634.0 | -518.8 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -13.55 | 134.00 | 22.05 | 240.40 | 0.4216 | -806.0 | -583.9 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -14.02 | 133.88 | 21.93 | 239.28 | 0.4233 | -877.0 | -778.6 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -14.46 | 133.82 | 21.87 | 238.31 | 0.4257 | -830.0 | -709.5 | |
| 0.00 | 1.62 | 0.00 | 0.89 | -14.24 | 133.73 | 21.78 | 238.66 | 0.4229 | -821.0 | -642.9 | |
| 3.78 | 9.19 | 2.06 | 5.00 | -13.65 | 133.57 | 21.62 | 239.74 | 0.4164 | -1120.0 | -895.7 | |
| 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. | |