SDO HMI 2011-08-15 19:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.48 | 171.67 | 57.54 | 450.25 | 15.52 | 60.06 | -80.25 | 75.40 | 0.9801 | -260.0 | -27.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.94 | 95.65 | 10.89 | 181.76 | 16.03 | 64.76 | -75.55 | 75.17 | 0.9640 | -614.5 | -60.2 | |
| 2.61 | -1.00 | 4.87 | -1.00 | 15.66 | 64.53 | -75.78 | 75.54 | 0.9651 | -473.8 | 999999 | |
| 0.27 | -1.00 | 0.52 | -1.00 | 15.52 | 63.88 | -76.43 | 75.65 | 0.9679 | -3.7 | 999999 | |
| 4.86 | -1.00 | 9.52 | -1.00 | 15.47 | 63.67 | -76.64 | 75.70 | 0.9688 | 230.2 | 999999 | |
| 2.34 | -1.00 | 4.53 | -1.00 | 15.22 | 63.96 | -76.35 | 75.97 | 0.9676 | -179.7 | 999999 | |
| 2.70 | 20.72 | 6.74 | 53.48 | 16.56 | 60.38 | -79.93 | 74.40 | 0.9808 | -260.7 | 172.1 | |
| 0.27 | -6.00 | 0.68 | -6.00 | 16.26 | 60.32 | -79.99 | 74.69 | 0.9810 | 227.7 | 999999 | |
| 0.00 | 10.00 | 0.00 | 41.44 | 18.17 | 55.49 | -84.82 | 72.42 | 0.9931 | 202.0 | 180.0 | |
| 0.00 | 2.16 | 0.00 | 5.65 | 15.42 | 59.84 | -80.47 | 75.52 | 0.9828 | 400.0 | 434.6 | |
| 1.26 | 3.24 | 3.34 | 8.46 | 15.15 | 59.70 | -80.61 | 75.78 | 0.9833 | 524.6 | 470.9 | |
| 0.00 | 1.44 | 0.00 | 5.18 | 15.94 | 56.62 | -83.69 | 74.75 | 0.9912 | 164.0 | 141.6 | |
| 0.00 | 1.17 | 0.00 | 3.03 | 13.90 | 60.11 | -80.20 | 77.08 | 0.9823 | 379.0 | 344.4 | |
| 4.23 | 37.29 | 16.45 | 151.25 | 14.29 | 56.32 | -83.99 | 76.39 | 0.9922 | -588.0 | -175.4 | |
| 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. | |