SDO HMI 2014-10-09 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.36 | 0.00 | 11.65 | 14.17 | 89.02 | 14.79 | 302.43 | 0.2973 | 136.9 | 281.6 | |
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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 | 1.14 | 0.00 | 0.65 | 9.32 | 104.26 | 30.03 | 277.82 | 0.5005 | -569.0 | -508.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 11.29 | 98.62 | 24.39 | 283.50 | 0.4182 | -836.0 | -615.8 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 12.15 | 98.33 | 24.10 | 285.66 | 0.4163 | -695.0 | -481.4 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 7.34 | 96.12 | 21.89 | 274.13 | 0.3723 | -923.0 | -702.1 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 8.32 | 95.76 | 21.52 | 276.82 | 0.3672 | -831.0 | -692.4 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 15.66 | 88.17 | 13.94 | 305.66 | 0.2867 | 793.0 | 703.8 | |
| 0.00 | 2.89 | 0.00 | 1.50 | 15.94 | 87.90 | 13.67 | 306.98 | 0.2857 | 947.0 | 726.6 | |
| 0.00 | 4.21 | 0.00 | 2.16 | 14.17 | 87.31 | 13.07 | 302.60 | 0.2615 | 779.0 | 705.6 | |
| 0.00 | 2.37 | 0.00 | 1.22 | 14.75 | 86.96 | 12.73 | 305.18 | 0.2619 | 893.0 | 853.7 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 14.67 | 86.58 | 12.34 | 305.71 | 0.2558 | 826.0 | 649.0 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 18.97 | 86.55 | 12.31 | 317.79 | 0.3015 | 829.0 | 613.7 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 16.77 | 84.76 | 10.53 | 316.48 | 0.2552 | 861.0 | 752.2 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 23.76 | 82.88 | 8.64 | 335.51 | 0.3332 | 686.0 | 568.3 | |
| 0.00 | 2.28 | 0.00 | 1.14 | 11.88 | 81.00 | 6.77 | 310.54 | 0.1524 | -843.0 | -557.3 | |
| 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. | |