SDO HMI 2011-04-30 16:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.44 | 28.08 | 2.96 | 15.08 | 17.28 | 111.80 | -5.78 | 14.51 | 0.3808 | -406.5 | -304.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.62 | 19.02 | 115.67 | -1.91 | 4.56 | 0.3978 | 699.0 | 496.8 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 11.05 | 114.57 | -3.01 | 11.06 | 0.2698 | -880.0 | -691.7 | |
| 0.00 | 2.41 | 0.00 | 1.26 | 14.46 | 114.03 | -3.55 | 10.60 | 0.3275 | -811.0 | -737.3 | |
| 1.69 | 2.67 | 0.89 | 1.40 | 14.69 | 113.49 | -4.09 | 12.00 | 0.3329 | -909.2 | -707.1 | |
| 0.00 | 2.85 | 0.00 | 1.50 | 14.46 | 113.19 | -4.39 | 13.03 | 0.3305 | -981.0 | -693.1 | |
| 0.00 | 1.43 | 0.00 | 0.75 | 13.99 | 113.01 | -4.57 | 13.90 | 0.3235 | -860.0 | -650.8 | |
| 0.00 | 2.05 | 0.00 | 1.07 | 14.21 | 112.66 | -4.92 | 14.73 | 0.3285 | -942.0 | -682.7 | |
| 0.00 | 1.34 | 0.00 | 0.71 | 15.65 | 112.22 | -5.36 | 14.82 | 0.3533 | -514.0 | -455.1 | |
| 2.32 | 5.08 | 1.28 | 2.81 | 21.33 | 111.12 | -6.46 | 13.65 | 0.4457 | -892.7 | -604.8 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 13.12 | 110.66 | -6.92 | 21.51 | 0.3216 | -846.0 | -645.3 | |
| 1.43 | 4.46 | 0.79 | 2.48 | 21.71 | 110.22 | -7.36 | 15.23 | 0.4549 | 581.6 | 724.2 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 11.44 | 108.24 | -9.34 | 30.54 | 0.3142 | -744.0 | -643.6 | |
| 0.00 | 0.62 | 0.00 | 0.35 | 21.66 | 105.91 | -11.67 | 23.35 | 0.4763 | 824.0 | 703.4 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 20.60 | 105.50 | -12.08 | 25.08 | 0.4641 | 873.0 | 690.5 | |
| 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. | |