SDO HMI 2011-08-31 02:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.61 | 278.73 | 22.39 | 140.00 | 13.88 | 291.58 | -6.66 | 43.76 | 0.1638 | -661.1 | -336.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.52 | 0.00 | 0.76 | 14.90 | 295.32 | -2.92 | 20.13 | 0.1439 | -811.0 | -558.1 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 9.66 | 293.78 | -4.47 | 60.37 | 0.0887 | -904.0 | -647.2 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 18.41 | 293.19 | -5.06 | 23.19 | 0.2133 | 943.0 | 738.4 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 18.69 | 292.99 | -5.26 | 23.46 | 0.2190 | 678.0 | 496.6 | |
| 12.45 | 258.06 | 6.24 | 129.53 | 13.53 | 291.87 | -6.37 | 44.13 | 0.1557 | -1414.9 | -420.8 | |
| 2.15 | -5.00 | 1.08 | -5.00 | 14.29 | 291.85 | -6.39 | 40.93 | 0.1655 | -1138.8 | 999999 | |
| 30.01 | -5.00 | 15.07 | -5.00 | 13.92 | 291.64 | -6.60 | 43.38 | 0.1632 | -1297.3 | 999999 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 12.51 | 289.55 | -8.69 | 57.40 | 0.1759 | 923.0 | 750.8 | |
| 0.00 | 4.30 | 0.00 | 2.17 | 13.61 | 289.32 | -8.92 | 53.05 | 0.1894 | 979.0 | 761.5 | |
| 0.00 | 3.40 | 0.00 | 1.72 | 14.70 | 289.06 | -9.18 | 49.39 | 0.2043 | 732.0 | 649.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 13.93 | 288.93 | -9.31 | 52.81 | 0.1980 | 967.0 | 785.2 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 11.47 | 289.02 | -9.22 | 64.06 | 0.1754 | 959.0 | 752.9 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 15.02 | 287.01 | -11.24 | 53.61 | 0.2348 | 779.0 | 626.6 | |
| 0.00 | 1.61 | 0.00 | 0.83 | 16.79 | 286.58 | -11.66 | 48.81 | 0.2583 | 900.0 | 742.6 | |
| 0.00 | 1.34 | 0.00 | 0.69 | 15.73 | 285.88 | -12.37 | 53.71 | 0.2569 | 727.0 | 604.1 | |
| 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. | |