SDO HMI 2011-08-09 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.71 | 25.26 | 0.87 | 12.90 | 19.60 | 224.39 | 4.75 | 341.44 | 0.2454 | -752.7 | -640.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.88 | 20.09 | 226.86 | 7.23 | 333.65 | 0.2675 | -742.0 | -589.4 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 19.94 | 226.69 | 7.06 | 333.91 | 0.2640 | -945.0 | -743.5 | |
| 0.00 | 2.17 | 0.00 | 1.11 | 19.57 | 225.93 | 6.30 | 335.76 | 0.2530 | -1120.0 | -938.6 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 19.95 | 225.59 | 5.96 | 337.54 | 0.2565 | -1020.0 | -846.6 | |
| 0.00 | 2.53 | 0.00 | 1.29 | 19.76 | 225.45 | 5.82 | 337.71 | 0.2527 | -817.0 | -786.8 | |
| 0.00 | 3.25 | 0.00 | 1.67 | 20.17 | 225.37 | 5.74 | 338.62 | 0.2586 | -787.0 | -729.9 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 19.67 | 225.32 | 5.69 | 338.02 | 0.2505 | -981.0 | -811.7 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 18.09 | 224.43 | 4.80 | 338.72 | 0.2201 | -812.0 | -751.8 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 18.34 | 224.18 | 4.55 | 340.14 | 0.2226 | -903.0 | -778.5 | |
| 0.00 | 2.35 | 0.00 | 1.19 | 18.56 | 223.77 | 4.14 | 342.13 | 0.2239 | -817.0 | -709.4 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.28 | 223.70 | 4.07 | 342.01 | 0.2190 | -1003.0 | -827.5 | |
| 0.00 | 3.34 | 0.00 | 1.71 | 20.85 | 221.88 | 2.24 | 351.70 | 0.2546 | -537.0 | -406.9 | |
| 1.71 | 2.80 | 0.87 | 1.42 | 19.14 | 221.47 | 1.83 | 352.24 | 0.2247 | 915.5 | 955.8 | |
| 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. | |