SDO HMI 2011-08-28 14:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.61 | 250.74 | 21.58 | 161.72 | 13.46 | 291.37 | -39.91 | 77.47 | 0.6413 | -438.1 | -223.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.31 | 227.15 | 18.78 | 145.85 | 13.44 | 291.76 | -39.52 | 77.45 | 0.6363 | -1014.4 | -320.5 | |
| 1.88 | -1.00 | 1.21 | -1.00 | 13.58 | 291.25 | -40.04 | 77.29 | 0.6433 | -594.9 | 999999 | |
| 1.43 | -1.00 | 0.93 | -1.00 | 13.45 | 291.07 | -40.21 | 77.53 | 0.6454 | -565.9 | 999999 | |
| 0.00 | 1.52 | 0.00 | 1.00 | 11.90 | 290.14 | -41.15 | 80.00 | 0.6560 | 693.0 | 589.7 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 12.21 | 289.79 | -41.49 | 79.56 | 0.6607 | 515.0 | 388.7 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 13.26 | 289.46 | -41.83 | 78.01 | 0.6659 | 565.0 | 536.5 | |
| 0.00 | 2.78 | 0.00 | 1.86 | 13.22 | 288.58 | -42.71 | 78.16 | 0.6769 | 806.0 | 675.2 | |
| 0.99 | 8.52 | 0.66 | 5.72 | 13.57 | 288.46 | -42.83 | 77.65 | 0.6788 | 713.8 | 650.8 | |
| 0.00 | 1.61 | 0.00 | 1.09 | 13.46 | 288.18 | -43.10 | 77.85 | 0.6821 | 557.0 | 452.7 | |
| 0.00 | 1.08 | 0.00 | 0.73 | 14.09 | 288.04 | -43.25 | 76.93 | 0.6845 | 525.0 | 440.7 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 13.70 | 288.09 | -43.20 | 77.51 | 0.6835 | 547.0 | 477.2 | |
| 0.00 | 0.99 | 0.00 | 0.67 | 14.40 | 287.62 | -43.67 | 76.54 | 0.6900 | 538.0 | 430.6 | |
| 0.00 | 1.61 | 0.00 | 1.11 | 14.34 | 287.28 | -44.00 | 76.66 | 0.6940 | 599.0 | 571.1 | |
| 0.00 | 2.69 | 0.00 | 1.84 | 14.09 | 287.26 | -44.03 | 77.03 | 0.6940 | 646.0 | 545.5 | |
| 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. | |