SDO HMI 2011-08-09 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.63 | 28.37 | 0.32 | 14.44 | 19.28 | 224.65 | 1.70 | 353.17 | 0.2280 | -781.8 | -669.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.46 | 20.55 | 226.48 | 3.53 | 346.82 | 0.2539 | -736.0 | -595.0 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 20.70 | 226.29 | 3.34 | 347.65 | 0.2558 | -801.0 | -673.5 | |
| 0.63 | 3.07 | 0.32 | 1.57 | 19.58 | 225.95 | 2.99 | 347.92 | 0.2359 | -1130.3 | -867.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 20.64 | 225.93 | 2.98 | 348.89 | 0.2535 | -936.0 | -772.8 | |
| 0.00 | 5.78 | 0.00 | 2.95 | 19.92 | 225.60 | 2.64 | 349.58 | 0.2405 | -858.0 | -744.9 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.89 | 225.18 | 2.22 | 351.19 | 0.2388 | -952.0 | -748.5 | |
| 0.00 | 1.90 | 0.00 | 0.96 | 18.18 | 224.32 | 1.37 | 353.72 | 0.2080 | -944.0 | -803.3 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 18.49 | 224.29 | 1.34 | 354.02 | 0.2132 | -1009.0 | -799.9 | |
| 0.00 | 2.26 | 0.00 | 1.15 | 19.21 | 224.27 | 1.31 | 354.48 | 0.2253 | -879.0 | -691.8 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 18.99 | 224.23 | 1.28 | 354.52 | 0.2216 | -1074.0 | -876.1 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 18.65 | 223.49 | 0.54 | 357.63 | 0.2149 | -734.0 | -549.8 | |
| 0.00 | 4.97 | 0.00 | 2.52 | 18.31 | 223.43 | 0.47 | 357.85 | 0.2090 | -964.0 | -859.5 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 19.02 | 221.63 | -1.33 | 5.68 | 0.2222 | 965.0 | 907.4 | |
| 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. | |