SDO HMI 2014-08-05 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.02 | 0.00 | 11.66 | -19.35 | 238.63 | 25.93 | 224.40 | 0.5910 | -85.3 | -78.0 | |
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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 | 1.00 | 0.00 | 0.63 | -17.51 | 243.07 | 30.36 | 231.30 | 0.6200 | 837.0 | 621.4 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -17.95 | 242.08 | 29.37 | 229.81 | 0.6131 | 626.0 | 484.9 | |
| 0.00 | 1.27 | 0.00 | 0.79 | -18.07 | 241.11 | 28.41 | 228.74 | 0.6039 | 688.0 | 530.3 | |
| 0.00 | 1.72 | 0.00 | 1.07 | -19.35 | 240.87 | 28.17 | 226.85 | 0.6127 | 689.0 | 517.8 | |
| 0.00 | 1.00 | 0.00 | 0.64 | -21.65 | 241.30 | 28.59 | 224.47 | 0.6373 | 501.0 | 451.5 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -19.74 | 240.61 | 27.91 | 226.10 | 0.6136 | 592.0 | 467.9 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -19.89 | 240.17 | 27.46 | 225.47 | 0.6105 | 594.0 | 573.6 | |
| 0.00 | 2.35 | 0.00 | 1.43 | -19.16 | 237.70 | 24.99 | 223.75 | 0.5793 | -734.0 | -459.3 | |
| 0.00 | 1.09 | 0.00 | 0.67 | -20.74 | 237.50 | 24.79 | 221.59 | 0.5930 | -674.0 | -533.7 | |
| 0.00 | 2.26 | 0.00 | 1.38 | -20.04 | 237.13 | 24.42 | 222.01 | 0.5826 | -813.0 | -671.9 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -18.38 | 236.76 | 24.06 | 223.68 | 0.5624 | -679.0 | -587.2 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -20.13 | 236.86 | 24.15 | 221.59 | 0.5809 | -646.0 | -523.8 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -19.67 | 234.85 | 22.15 | 219.74 | 0.5573 | -721.0 | -593.2 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -19.48 | 234.41 | 21.70 | 219.41 | 0.5512 | -755.0 | -602.6 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -18.69 | 234.09 | 21.39 | 219.98 | 0.5397 | -785.0 | -611.3 | |
| 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. | |