SDO HMI 2011-08-05 01:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.60 | 29.58 | 4.32 | 19.51 | 18.44 | 242.08 | -40.36 | 68.75 | 0.6607 | -78.4 | 165.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 3.53 | 0.34 | 2.20 | 18.19 | 246.25 | -36.19 | 67.74 | 0.6083 | -923.7 | -768.4 | |
| 0.00 | 1.27 | 0.00 | 0.79 | 17.59 | 246.19 | -36.25 | 68.72 | 0.6071 | -780.0 | -585.5 | |
| 0.00 | 1.54 | 0.00 | 0.97 | 17.92 | 245.55 | -36.88 | 68.42 | 0.6163 | -623.0 | -613.2 | |
| 0.00 | 0.81 | 0.00 | 0.51 | 17.94 | 245.35 | -37.09 | 68.46 | 0.6190 | -482.0 | -404.3 | |
| 3.98 | 6.06 | 2.59 | 3.95 | 18.26 | 242.89 | -39.54 | 68.81 | 0.6507 | -746.8 | -579.3 | |
| 0.45 | -5.00 | 0.29 | -5.00 | 18.44 | 242.84 | -39.59 | 68.55 | 0.6519 | -612.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.92 | 19.17 | 240.46 | -41.98 | 68.22 | 0.6827 | 605.0 | 572.5 | |
| 1.09 | 1.90 | 0.73 | 1.28 | 18.95 | 240.48 | -41.95 | 68.52 | 0.6818 | 858.4 | 823.1 | |
| 0.00 | 2.53 | 0.00 | 1.70 | 18.18 | 240.71 | -41.72 | 69.57 | 0.6770 | 729.0 | 664.4 | |
| 0.00 | 1.72 | 0.00 | 1.16 | 18.78 | 240.40 | -42.03 | 68.78 | 0.6823 | 531.0 | 485.6 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 18.38 | 240.48 | -41.95 | 69.34 | 0.6803 | 386.0 | 316.1 | |
| 0.54 | 5.88 | 0.37 | 4.00 | 18.79 | 240.01 | -42.43 | 68.88 | 0.6870 | 844.8 | 583.1 | |
| 0.00 | 2.17 | 0.00 | 1.48 | 18.32 | 239.59 | -42.85 | 69.67 | 0.6908 | 611.0 | 578.5 | |
| 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. | |