SDO HMI 2011-09-02 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 |
| 26.04 | 142.50 | 13.99 | 76.30 | 13.74 | 291.49 | 21.86 | 288.84 | 0.3838 | -523.0 | -455.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.24 | 14.27 | 293.50 | 23.87 | 288.78 | 0.4159 | -505.0 | -445.8 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 14.28 | 293.33 | 23.70 | 288.90 | 0.4134 | -842.0 | -693.7 | |
| 1.07 | 128.00 | 0.58 | 68.65 | 13.00 | 292.08 | 22.45 | 286.48 | 0.3897 | -859.8 | -581.5 | |
| 5.46 | -3.00 | 2.93 | -3.00 | 13.24 | 292.04 | 22.40 | 287.13 | 0.3899 | -1080.5 | 999999 | |
| 6.44 | -3.00 | 3.47 | -3.00 | 14.01 | 291.91 | 22.28 | 289.12 | 0.3910 | -971.0 | 999999 | |
| 11.01 | -3.00 | 5.91 | -3.00 | 13.56 | 291.73 | 22.10 | 288.11 | 0.3864 | -1126.4 | 999999 | |
| 2.06 | -3.00 | 1.10 | -3.00 | 13.23 | 291.70 | 22.07 | 287.28 | 0.3846 | -1145.7 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 13.54 | 290.86 | 21.23 | 288.61 | 0.3730 | -932.0 | -730.8 | |
| 0.00 | 2.33 | 0.00 | 1.22 | 14.72 | 288.05 | 18.41 | 294.16 | 0.3363 | 730.0 | 584.4 | |
| 0.00 | 3.40 | 0.00 | 1.79 | 14.89 | 287.80 | 18.16 | 294.87 | 0.3335 | 945.0 | 783.2 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 16.32 | 287.03 | 17.40 | 299.73 | 0.3320 | 827.0 | 624.7 | |
| 0.00 | 2.15 | 0.00 | 1.13 | 16.11 | 286.98 | 17.35 | 299.22 | 0.3297 | 911.0 | 622.8 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 17.74 | 286.87 | 17.24 | 303.70 | 0.3407 | 807.0 | 617.9 | |
| 0.00 | 2.06 | 0.00 | 1.08 | 16.64 | 286.73 | 17.10 | 300.99 | 0.3301 | 986.0 | 753.2 | |
| 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. | |