SDO HMI 2014-11-10 08:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.76 | 0.00 | 9.90 | -23.60 | 9.02 | -3.73 | 172.58 | 0.4598 | 704.8 | 644.3 | |
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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 | 0.95 | 0.00 | 0.52 | -20.75 | 10.22 | -2.54 | 174.21 | 0.4129 | 726.0 | 578.7 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -21.34 | 10.17 | -2.58 | 174.27 | 0.4222 | 929.0 | 781.5 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -22.55 | 10.02 | -2.74 | 174.25 | 0.4416 | 690.0 | 508.4 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -22.46 | 9.83 | -2.93 | 173.82 | 0.4404 | 877.0 | 707.0 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -22.72 | 9.44 | -3.32 | 173.08 | 0.4452 | 781.0 | 659.9 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -24.02 | 9.11 | -3.65 | 172.81 | 0.4659 | 889.0 | 796.5 | |
| 0.00 | 3.45 | 0.00 | 1.94 | -24.73 | 8.99 | -3.77 | 172.78 | 0.4770 | 705.0 | 604.5 | |
| 0.00 | 1.55 | 0.00 | 0.87 | -24.39 | 9.00 | -3.76 | 172.71 | 0.4718 | 881.0 | 778.5 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.22 | 8.87 | -3.88 | 172.41 | 0.4695 | 836.0 | 757.0 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -25.27 | 8.54 | -4.21 | 172.12 | 0.4861 | 699.0 | 601.1 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -23.96 | 8.33 | -4.43 | 171.27 | 0.4666 | 738.0 | 690.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.03 | 7.77 | -4.98 | 170.22 | 0.4691 | 707.0 | 618.2 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -25.02 | 4.76 | -7.99 | 165.15 | 0.4938 | -295.0 | -321.4 | |
| 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. | |