SDO HMI 2012-05-07 06:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.64 | 35.90 | 2.98 | 19.27 | 15.14 | 227.23 | -12.54 | 32.63 | 0.3828 | 10.6 | 2.7 | |
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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 | 1.61 | 0.00 | 0.84 | 12.91 | 234.18 | -5.59 | 18.62 | 0.2987 | 925.0 | 696.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 11.56 | 233.93 | -5.84 | 21.04 | 0.2789 | -772.0 | -590.6 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 11.66 | 233.24 | -6.53 | 23.12 | 0.2847 | -775.0 | -599.4 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 14.40 | 230.43 | -9.34 | 27.19 | 0.3457 | -584.0 | -604.2 | |
| 3.31 | 14.59 | 1.75 | 7.69 | 13.77 | 229.47 | -10.30 | 30.43 | 0.3443 | -1001.3 | -887.7 | |
| 2.33 | -5.00 | 1.23 | -5.00 | 13.52 | 229.42 | -10.35 | 30.94 | 0.3412 | -1057.3 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 13.82 | 228.14 | -11.63 | 33.47 | 0.3565 | -1019.0 | -784.2 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 13.79 | 227.82 | -11.95 | 34.23 | 0.3590 | -805.0 | -667.9 | |
| 0.00 | 1.43 | 0.00 | 0.78 | 16.90 | 225.27 | -14.51 | 34.68 | 0.4229 | 687.0 | 590.6 | |
| 0.00 | 2.33 | 0.00 | 1.27 | 16.97 | 224.80 | -14.97 | 35.42 | 0.4281 | 683.0 | 659.7 | |
| 0.00 | 3.13 | 0.00 | 1.72 | 17.33 | 224.38 | -15.39 | 35.66 | 0.4365 | 823.0 | 695.4 | |
| 0.00 | 1.61 | 0.00 | 0.90 | 17.69 | 222.86 | -16.91 | 37.71 | 0.4550 | 873.0 | 722.9 | |
| 0.00 | 1.97 | 0.00 | 1.10 | 17.91 | 222.77 | -17.00 | 37.53 | 0.4586 | 871.0 | 726.8 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 17.23 | 222.80 | -16.97 | 38.45 | 0.4502 | 881.0 | 758.2 | |
| 0.00 | 2.33 | 0.00 | 1.29 | 17.59 | 222.67 | -17.10 | 38.15 | 0.4557 | 723.0 | 601.1 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 17.60 | 220.43 | -19.34 | 41.54 | 0.4781 | 722.0 | 603.9 | |
| 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. | |