SDO HMI 2011-10-21 23:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.01 | 0.00 | 10.55 | 24.64 | 329.99 | -3.58 | 8.92 | 0.3406 | -464.7 | -462.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.26 | 0.00 | 1.18 | 23.24 | 336.36 | 2.79 | 351.72 | 0.3117 | -848.0 | -660.3 | |
| 0.00 | 1.57 | 0.00 | 0.83 | 25.33 | 333.14 | -0.43 | 1.15 | 0.3430 | -901.0 | -689.9 | |
| 0.00 | 1.74 | 0.00 | 0.89 | 20.54 | 333.12 | -0.45 | 1.61 | 0.2630 | -900.0 | -685.8 | |
| 0.00 | 1.39 | 0.00 | 0.72 | 22.74 | 330.91 | -2.66 | 8.14 | 0.3031 | -899.0 | -739.0 | |
| 0.00 | 1.83 | 0.00 | 0.96 | 24.88 | 329.72 | -3.85 | 10.34 | 0.3412 | -783.0 | -648.5 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 25.26 | 329.60 | -3.96 | 10.41 | 0.3476 | -647.0 | -495.0 | |
| 0.00 | 3.05 | 0.00 | 1.61 | 25.10 | 329.51 | -4.06 | 10.74 | 0.3453 | -826.0 | -666.5 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 24.75 | 329.49 | -4.08 | 11.01 | 0.3398 | -904.0 | -789.3 | |
| 0.00 | 1.48 | 0.00 | 0.78 | 24.43 | 329.47 | -4.10 | 11.27 | 0.3348 | -946.0 | -781.2 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 27.01 | 329.27 | -4.29 | 10.24 | 0.3767 | -765.0 | -639.1 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 27.61 | 325.22 | -8.35 | 18.73 | 0.4024 | 774.0 | 600.9 | |
| 0.00 | 1.39 | 0.00 | 0.75 | 26.13 | 322.73 | -10.83 | 25.36 | 0.3957 | 877.0 | 674.1 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 26.29 | 322.69 | -10.88 | 25.27 | 0.3983 | 727.0 | 577.6 | |
| 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. | |