SDO HMI 2014-04-24 05:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.27 | 0.00 | 9.27 | -18.66 | 163.24 | 25.70 | 239.21 | 0.4855 | -581.9 | -509.0 | |
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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 | 0.98 | 0.00 | 0.67 | -17.74 | 179.77 | 42.22 | 249.13 | 0.6873 | 519.0 | 431.9 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -27.97 | 169.92 | 32.37 | 229.46 | 0.6244 | -615.0 | -501.8 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -13.12 | 162.36 | 24.81 | 249.66 | 0.4376 | -642.0 | -518.2 | |
| 0.00 | 2.22 | 0.00 | 1.21 | -9.83 | 161.52 | 23.97 | 256.77 | 0.4129 | -934.0 | -819.2 | |
| 0.00 | 4.00 | 0.00 | 2.23 | -17.24 | 162.14 | 24.60 | 240.82 | 0.4572 | -737.0 | -617.3 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -17.06 | 161.95 | 24.40 | 241.00 | 0.4533 | -810.0 | -658.0 | |
| 0.00 | 1.96 | 0.00 | 1.08 | -16.98 | 161.62 | 24.07 | 240.89 | 0.4484 | -578.0 | -525.4 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -19.74 | 161.79 | 24.24 | 235.65 | 0.4700 | -610.0 | -502.0 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -23.85 | 160.87 | 23.33 | 227.49 | 0.4933 | -652.0 | -488.7 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -24.78 | 160.84 | 23.29 | 225.95 | 0.5015 | -654.0 | -463.7 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -24.19 | 159.08 | 21.53 | 224.83 | 0.4767 | -682.0 | -488.6 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -26.22 | 159.06 | 21.51 | 221.65 | 0.4970 | -588.0 | -468.6 | |
| 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. | |