SDO HMI 2011-08-27 21:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.16 | 51.92 | 10.90 | 26.70 | 17.76 | 329.05 | -11.58 | 45.40 | 0.2701 | 28.3 | -89.7 | |
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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 | 18.65 | 332.92 | -7.70 | 32.28 | 0.2389 | -718.0 | -482.3 | |
| 0.00 | 3.41 | 0.00 | 1.74 | 18.26 | 331.78 | -8.85 | 36.86 | 0.2445 | -1001.0 | -854.8 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 17.42 | 331.82 | -8.80 | 38.97 | 0.2332 | -901.0 | -715.7 | |
| 0.00 | 3.41 | 0.00 | 1.74 | 18.07 | 331.53 | -9.09 | 38.11 | 0.2446 | -785.0 | -626.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 18.03 | 331.11 | -9.51 | 39.43 | 0.2485 | -906.0 | -774.8 | |
| 0.00 | 1.88 | 0.00 | 0.96 | 17.38 | 331.15 | -9.48 | 41.12 | 0.2400 | -1019.0 | -754.4 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 19.49 | 328.84 | -11.79 | 41.59 | 0.2914 | -758.0 | -535.2 | |
| 7.89 | 12.91 | 4.08 | 6.67 | 19.09 | 328.74 | -11.89 | 42.81 | 0.2877 | -994.9 | -616.4 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 18.10 | 328.64 | -11.98 | 45.60 | 0.2774 | 1158.0 | 873.7 | |
| 7.26 | 19.72 | 3.73 | 10.14 | 17.14 | 328.51 | -12.11 | 48.59 | 0.2685 | 1096.7 | 784.3 | |
| 6.01 | -10.00 | 3.09 | -10.00 | 16.88 | 328.24 | -12.38 | 49.94 | 0.2694 | 1033.7 | 999999 | |
| 0.00 | 2.42 | 0.00 | 1.25 | 15.09 | 326.58 | -14.04 | 58.69 | 0.2754 | 931.0 | 768.3 | |
| 0.00 | 0.36 | 0.00 | 0.18 | 14.74 | 326.09 | -14.54 | 60.62 | 0.2798 | 658.0 | 782.2 | |
| 0.00 | 1.34 | 0.00 | 0.70 | 17.31 | 324.91 | -15.72 | 54.92 | 0.3174 | 736.0 | 494.1 | |
| 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. | |