SDO HMI 2011-08-28 16:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.95 | 0.00 | 14.46 | 7.53 | 346.48 | 16.30 | 272.73 | 0.2793 | -37.1 | -105.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.52 | 7.50 | 351.51 | 21.33 | 272.41 | 0.3626 | -766.0 | -663.3 | |
| 0.00 | 2.15 | 0.00 | 1.14 | 7.72 | 351.36 | 21.18 | 273.01 | 0.3601 | -987.0 | -772.1 | |
| 0.00 | 3.23 | 0.00 | 1.71 | 7.41 | 351.31 | 21.13 | 272.17 | 0.3593 | -853.0 | -780.4 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 6.52 | 351.07 | 20.89 | 269.63 | 0.3559 | -756.0 | -673.4 | |
| 0.00 | 2.51 | 0.00 | 1.33 | 7.73 | 351.10 | 20.92 | 273.05 | 0.3558 | -504.0 | -685.0 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 7.52 | 346.22 | 16.04 | 272.50 | 0.2755 | -856.0 | -649.5 | |
| 0.00 | 1.43 | 0.00 | 0.74 | 7.80 | 346.04 | 15.86 | 273.54 | 0.2726 | -1007.0 | -775.3 | |
| 0.00 | 1.34 | 0.00 | 0.69 | 8.29 | 346.03 | 15.85 | 275.32 | 0.2727 | -831.0 | -715.9 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 8.85 | 343.52 | 13.34 | 278.39 | 0.2315 | 598.0 | 469.4 | |
| 0.00 | 3.41 | 0.00 | 1.73 | 7.26 | 342.84 | 12.66 | 271.49 | 0.2185 | 744.0 | 550.4 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 7.42 | 342.63 | 12.45 | 272.22 | 0.2149 | 848.0 | 714.7 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 6.73 | 342.55 | 12.37 | 268.96 | 0.2137 | 1025.0 | 787.1 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 7.12 | 342.56 | 12.38 | 270.81 | 0.2137 | 916.0 | 776.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 7.24 | 342.43 | 12.26 | 271.39 | 0.2116 | 910.0 | 745.7 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 8.59 | 339.27 | 9.09 | 279.91 | 0.1593 | 962.0 | 728.4 | |
| 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. | |