SDO HMI 2011-08-25 13:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 21.29 | 0.24 | 14.26 | 16.99 | 329.27 | -42.20 | 72.39 | 0.6759 | -167.0 | -48.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.27 | 0.00 | 0.17 | 23.51 | 333.18 | -38.29 | 61.55 | 0.6485 | 578.0 | 621.0 | |
| 0.00 | 0.72 | 0.00 | 0.45 | 15.20 | 333.56 | -37.92 | 74.27 | 0.6183 | -742.0 | -581.0 | |
| 0.00 | 1.35 | 0.00 | 0.85 | 15.25 | 332.99 | -38.49 | 74.31 | 0.6259 | -583.0 | -456.5 | |
| 0.00 | 1.44 | 0.00 | 0.91 | 14.30 | 333.14 | -38.33 | 75.79 | 0.6222 | -570.0 | -423.6 | |
| 0.00 | 2.15 | 0.00 | 1.40 | 17.50 | 331.63 | -39.85 | 71.13 | 0.6481 | -666.0 | -607.8 | |
| 0.00 | 0.81 | 0.00 | 0.52 | 17.68 | 331.58 | -39.89 | 70.86 | 0.6491 | -619.0 | -524.2 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 19.14 | 331.00 | -40.47 | 68.83 | 0.6599 | -542.0 | -463.4 | |
| 0.00 | 3.50 | 0.00 | 2.32 | 18.52 | 330.38 | -41.10 | 69.91 | 0.6659 | -571.0 | -397.9 | |
| 0.36 | 1.08 | 0.24 | 0.73 | 18.69 | 328.55 | -42.92 | 70.12 | 0.6882 | -586.0 | -510.1 | |
| 0.00 | 1.26 | 0.00 | 0.86 | 18.26 | 328.21 | -43.27 | 70.82 | 0.6914 | -551.0 | -461.3 | |
| 0.00 | 0.99 | 0.00 | 0.68 | 16.14 | 327.07 | -44.40 | 74.06 | 0.7013 | 695.0 | 552.9 | |
| 0.00 | 3.05 | 0.00 | 2.14 | 16.79 | 326.34 | -45.13 | 73.25 | 0.7108 | 664.0 | 565.9 | |
| 0.00 | 3.32 | 0.00 | 2.32 | 16.00 | 326.49 | -44.98 | 74.35 | 0.7080 | 748.0 | 583.3 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 14.56 | 325.90 | -45.57 | 76.45 | 0.7133 | 508.0 | 496.6 | |
| 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. | |