SDO HMI 2014-04-05 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.58 | 0.00 | 8.99 | 5.05 | 24.55 | -6.62 | 29.02 | 0.2325 | -25.3 | 10.2 | |
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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 | 1.23 | 0.00 | 0.62 | 3.40 | 28.28 | -2.88 | 16.52 | 0.1771 | -833.0 | -637.1 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 3.49 | 28.10 | -3.06 | 17.34 | 0.1795 | -841.0 | -754.1 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 3.04 | 27.98 | -3.18 | 18.79 | 0.1727 | -893.0 | -724.7 | |
| 0.00 | 1.49 | 0.00 | 0.75 | 3.40 | 27.89 | -3.27 | 18.61 | 0.1792 | -654.0 | -508.8 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 3.10 | 27.74 | -3.42 | 19.98 | 0.1751 | -813.0 | -695.2 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 4.30 | 26.08 | -5.08 | 25.61 | 0.2052 | -711.0 | -565.4 | |
| 0.00 | 1.05 | 0.00 | 0.53 | -2.08 | 25.97 | -5.20 | 50.79 | 0.1174 | 838.0 | 617.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 1.54 | 25.70 | -5.46 | 34.86 | 0.1673 | -828.0 | -654.7 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 7.39 | 24.23 | -6.93 | 26.82 | 0.2663 | 860.0 | 677.5 | |
| 0.00 | 2.73 | 0.00 | 1.41 | 8.17 | 24.04 | -7.12 | 26.18 | 0.2795 | 611.0 | 456.6 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 9.39 | 21.78 | -9.39 | 30.83 | 0.3154 | 659.0 | 571.3 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 9.27 | 21.66 | -9.51 | 31.36 | 0.3147 | 690.0 | 603.8 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 5.09 | 17.16 | -14.01 | 51.04 | 0.3114 | 931.0 | 829.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 6.48 | 16.87 | -14.29 | 48.30 | 0.3299 | 630.0 | 588.5 | |
| 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. | |