SDO HMI 2014-10-13 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.90 | 315.11 | 52.72 | 335.25 | -8.94 | 318.76 | -60.51 | 103.48 | 0.8836 | 484.7 | 177.8 | |
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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 |
| 14.17 | 268.77 | 13.97 | 266.50 | -8.52 | 321.07 | -58.21 | 103.49 | 0.8665 | 796.3 | 201.2 | |
| 29.82 | -1.00 | 29.64 | -1.00 | -9.06 | 320.87 | -58.40 | 104.05 | 0.8691 | 651.3 | 999999 | |
| 2.36 | -1.00 | 2.35 | -1.00 | -8.36 | 320.76 | -58.52 | 103.24 | 0.8688 | 342.9 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.84 | -9.69 | 318.70 | -60.57 | 104.24 | 0.8877 | 237.0 | 229.9 | |
| 0.00 | 0.52 | 0.00 | 0.56 | -9.14 | 318.62 | -60.66 | 103.62 | 0.8874 | 166.0 | 229.0 | |
| 0.00 | 2.36 | 0.00 | 2.95 | -8.62 | 314.08 | -65.19 | 102.09 | 0.9195 | -504.0 | -462.6 | |
| 0.00 | 0.96 | 0.00 | 1.21 | -8.46 | 313.84 | -65.43 | 101.87 | 0.9209 | -369.0 | -334.9 | |
| 0.00 | 1.05 | 0.00 | 1.51 | -8.94 | 310.76 | -68.51 | 101.82 | 0.9406 | -290.0 | -312.4 | |
| 0.00 | 0.26 | 0.00 | 0.38 | -9.25 | 310.47 | -68.81 | 102.08 | 0.9426 | -375.0 | -332.7 | |
| 4.55 | 23.61 | 6.76 | 35.60 | -8.92 | 310.10 | -69.18 | 101.67 | 0.9444 | -195.5 | 152.0 | |
| 0.00 | 16.79 | 0.00 | 25.70 | -9.82 | 309.69 | -69.58 | 102.54 | 0.9474 | 172.0 | 136.9 | |
| 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. | |