SDO HMI 2014-11-27 02:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.04 | 29.95 | 8.24 | 31.07 | -23.77 | 94.13 | -57.81 | 118.19 | 0.8806 | -113.7 | -159.1 | |
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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 | 1.11 | 0.00 | 1.11 | -24.30 | 95.80 | -56.14 | 119.25 | 0.8695 | 295.0 | 341.6 | |
| 6.16 | 11.90 | 6.22 | 11.99 | -24.34 | 95.30 | -56.64 | 119.15 | 0.8733 | 254.4 | 269.3 | |
| 0.00 | 0.77 | 0.00 | 0.79 | -24.13 | 94.73 | -57.21 | 118.74 | 0.8770 | -47.0 | 42.1 | |
| 0.00 | 1.97 | 0.00 | 2.02 | -23.71 | 94.42 | -57.52 | 118.19 | 0.8783 | -476.0 | -411.4 | |
| 0.00 | 0.94 | 0.00 | 0.99 | -24.61 | 93.77 | -58.17 | 118.99 | 0.8851 | 61.0 | 116.0 | |
| 0.00 | 1.28 | 0.00 | 1.34 | -23.68 | 94.01 | -57.93 | 118.05 | 0.8813 | -441.0 | -402.9 | |
| 0.00 | 0.51 | 0.00 | 0.54 | -23.69 | 93.64 | -58.31 | 117.96 | 0.8840 | -501.0 | -499.8 | |
| 0.00 | 1.28 | 0.00 | 1.34 | -23.17 | 93.63 | -58.31 | 117.39 | 0.8829 | -440.0 | -448.3 | |
| 0.00 | 1.88 | 0.00 | 1.99 | -22.89 | 93.21 | -58.73 | 116.96 | 0.8854 | -521.0 | -408.7 | |
| 1.88 | 6.08 | 2.02 | 6.52 | -23.09 | 92.82 | -59.13 | 117.08 | 0.8887 | -458.1 | -392.7 | |
| 0.00 | 2.23 | 0.00 | 2.44 | -23.21 | 92.03 | -59.91 | 117.00 | 0.8945 | -548.0 | -364.7 | |
| 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. | |