SDO HMI 2011-10-23 14:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.17 | 0.00 | 7.80 | 23.40 | 331.25 | 19.09 | 316.71 | 0.4411 | -622.7 | -494.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.59 | 21.65 | 336.99 | 24.83 | 306.69 | 0.4887 | -705.0 | -494.8 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 22.19 | 335.78 | 23.62 | 308.87 | 0.4786 | -785.0 | -581.8 | |
| 0.00 | 1.13 | 0.00 | 0.62 | 21.45 | 332.61 | 20.45 | 311.23 | 0.4343 | -720.0 | -626.5 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 20.57 | 331.77 | 19.61 | 310.66 | 0.4161 | -876.0 | -621.6 | |
| 0.00 | 1.65 | 0.00 | 0.91 | 23.07 | 331.72 | 19.56 | 315.33 | 0.4400 | -814.0 | -635.3 | |
| 0.00 | 1.13 | 0.00 | 0.63 | 25.21 | 332.03 | 19.87 | 318.45 | 0.4656 | -734.0 | -511.8 | |
| 0.00 | 1.39 | 0.00 | 0.76 | 20.90 | 331.21 | 19.05 | 312.06 | 0.4124 | -789.0 | -580.0 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 23.52 | 330.48 | 18.32 | 317.84 | 0.4313 | -627.0 | -514.5 | |
| 0.00 | 1.13 | 0.00 | 0.62 | 24.75 | 330.39 | 18.23 | 320.01 | 0.4439 | -566.0 | -438.6 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 24.86 | 329.92 | 17.76 | 320.87 | 0.4404 | -728.0 | -560.9 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 24.30 | 329.63 | 17.47 | 320.40 | 0.4312 | -872.0 | -656.2 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 25.34 | 329.79 | 17.63 | 321.82 | 0.4446 | -654.0 | -565.8 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 26.76 | 323.01 | 10.85 | 335.50 | 0.4070 | 775.0 | 600.6 | |
| 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. | |