SDO HMI 2011-08-09 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.62 | 29.52 | 1.33 | 15.05 | 19.25 | 223.33 | 2.04 | 351.05 | 0.2327 | -504.3 | -607.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.57 | 225.94 | 4.65 | 341.62 | 0.2431 | -1250.0 | -983.8 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 19.73 | 225.62 | 4.33 | 343.00 | 0.2440 | -1038.0 | -830.8 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 19.92 | 225.53 | 4.23 | 343.58 | 0.2466 | -1013.0 | -908.7 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 20.20 | 225.37 | 4.08 | 344.47 | 0.2505 | -782.0 | -727.2 | |
| 0.00 | 2.35 | 0.00 | 1.20 | 19.95 | 225.27 | 3.98 | 344.56 | 0.2459 | -922.0 | -668.9 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 18.18 | 224.40 | 3.10 | 345.98 | 0.2131 | -916.0 | -764.4 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.40 | 224.37 | 3.07 | 346.36 | 0.2165 | -858.0 | -674.5 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 19.02 | 224.22 | 2.92 | 347.65 | 0.2263 | -1004.0 | -874.0 | |
| 0.00 | 2.35 | 0.00 | 1.19 | 18.37 | 224.11 | 2.82 | 347.42 | 0.2151 | -726.0 | -702.8 | |
| 0.00 | 8.31 | 0.00 | 4.21 | 18.37 | 223.60 | 2.30 | 349.66 | 0.2134 | -1031.0 | -682.6 | |
| 2.62 | 2.62 | 1.33 | 1.33 | 19.09 | 221.52 | 0.22 | 359.05 | 0.2222 | 907.7 | 0.0 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 21.03 | 214.74 | -6.56 | 22.72 | 0.2772 | 868.0 | 623.5 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 21.78 | 214.54 | -6.76 | 22.23 | 0.2900 | 742.0 | 615.7 | |
| 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. | |