SDO HMI 2011-08-09 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.72 | 26.08 | 0.37 | 13.32 | 19.24 | 224.40 | 5.32 | 338.88 | 0.2426 | -557.7 | -556.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.89 | 0.00 | 1.49 | 20.02 | 226.76 | 7.68 | 332.13 | 0.2699 | -831.0 | -717.9 | |
| 0.00 | 2.80 | 0.00 | 1.43 | 19.57 | 225.93 | 6.85 | 333.92 | 0.2568 | -1044.0 | -893.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 19.73 | 225.54 | 6.47 | 335.47 | 0.2565 | -948.0 | -797.4 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 19.82 | 225.42 | 6.34 | 336.05 | 0.2570 | -919.0 | -783.2 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 20.07 | 225.40 | 6.32 | 336.53 | 0.2607 | -998.0 | -842.5 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 19.67 | 225.25 | 6.17 | 336.35 | 0.2535 | -766.0 | -641.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 18.09 | 224.42 | 5.34 | 336.56 | 0.2235 | -851.0 | -733.7 | |
| 0.00 | 2.53 | 0.00 | 1.29 | 19.02 | 224.42 | 5.34 | 338.21 | 0.2381 | -677.0 | -613.1 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.37 | 224.37 | 5.29 | 337.29 | 0.2275 | -883.0 | -652.2 | |
| 0.00 | 2.26 | 0.00 | 1.15 | 18.50 | 223.82 | 4.75 | 339.61 | 0.2262 | -866.0 | -681.6 | |
| 0.00 | 2.53 | 0.00 | 1.28 | 18.22 | 223.75 | 4.67 | 339.44 | 0.2213 | -817.0 | -739.1 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 20.85 | 222.00 | 2.93 | 349.23 | 0.2565 | -798.0 | -639.6 | |
| 0.72 | 2.35 | 0.37 | 1.19 | 19.17 | 221.46 | 2.38 | 349.99 | 0.2266 | 1154.9 | 938.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 18.89 | 221.26 | 2.18 | 350.59 | 0.2214 | 801.0 | 647.8 | |
| 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. | |