SDO HMI 2014-07-08 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.89 | 177.14 | 17.52 | 94.72 | 6.67 | 203.98 | -21.90 | 81.17 | 0.3764 | -818.3 | -378.1 | |
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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 | 2.63 | 0.00 | 1.39 | 8.82 | 206.23 | -19.65 | 74.18 | 0.3469 | -927.0 | -666.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 5.88 | 205.80 | -20.07 | 82.80 | 0.3456 | -907.0 | -754.7 | |
| 6.45 | 8.99 | 3.42 | 4.77 | 7.15 | 205.29 | -20.58 | 79.37 | 0.3565 | -1088.5 | -719.0 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 11.36 | 204.37 | -21.51 | 68.87 | 0.3870 | -718.0 | -580.9 | |
| 25.53 | 147.98 | 13.61 | 78.88 | 6.37 | 204.34 | -21.54 | 81.86 | 0.3701 | -1395.5 | -414.7 | |
| 0.91 | -5.00 | 0.49 | -5.00 | 6.79 | 204.02 | -21.85 | 80.83 | 0.3760 | -620.4 | 999999 | |
| 0.00 | 1.73 | 0.00 | 0.93 | 9.04 | 203.57 | -22.31 | 75.20 | 0.3894 | -878.0 | -598.4 | |
| 0.00 | 3.00 | 0.00 | 1.61 | 8.51 | 203.17 | -22.71 | 76.74 | 0.3939 | -819.0 | -691.7 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 8.51 | 202.87 | -23.01 | 76.90 | 0.3986 | -707.0 | -527.4 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 8.04 | 197.81 | -28.07 | 79.75 | 0.4754 | 719.0 | 550.3 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 6.62 | 197.27 | -28.61 | 82.83 | 0.4813 | 778.0 | 536.0 | |
| 0.00 | 2.18 | 0.00 | 1.24 | 8.93 | 197.03 | -28.85 | 78.12 | 0.4890 | 107.0 | 242.6 | |
| 0.00 | 1.91 | 0.00 | 1.08 | 7.53 | 197.11 | -28.77 | 80.98 | 0.4851 | 718.0 | 552.6 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 6.80 | 197.16 | -28.72 | 82.48 | 0.4833 | 604.0 | 530.0 | |
| 0.00 | 1.64 | 0.00 | 0.93 | 9.05 | 196.74 | -29.14 | 77.98 | 0.4936 | 697.0 | 585.3 | |
| 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. | |