SDO HMI 2011-08-08 12:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.62 | 19.87 | 1.37 | 10.45 | 20.12 | 223.27 | -13.46 | 41.10 | 0.3290 | -604.4 | -450.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.33 | 19.18 | 226.24 | -10.49 | 37.33 | 0.2849 | -957.0 | -781.4 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 19.59 | 226.18 | -10.55 | 36.59 | 0.2907 | -969.0 | -728.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 19.80 | 225.97 | -10.76 | 36.66 | 0.2956 | -802.0 | -570.4 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 19.64 | 225.91 | -10.82 | 37.13 | 0.2941 | -963.0 | -746.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 18.49 | 225.99 | -10.74 | 39.58 | 0.2787 | -843.0 | -711.1 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 18.96 | 225.79 | -10.94 | 38.97 | 0.2866 | -815.0 | -720.5 | |
| 2.62 | 2.89 | 1.37 | 1.51 | 20.77 | 225.57 | -11.16 | 35.63 | 0.3121 | -887.0 | -862.3 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 20.45 | 225.43 | -11.31 | 36.61 | 0.3094 | -827.0 | -665.8 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 18.15 | 224.41 | -12.32 | 44.20 | 0.2922 | -873.0 | -666.5 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 18.90 | 223.20 | -13.53 | 44.94 | 0.3147 | -747.0 | -573.3 | |
| 0.00 | 3.16 | 0.00 | 1.68 | 20.89 | 221.55 | -15.18 | 43.67 | 0.3559 | -694.0 | -630.2 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 21.56 | 214.32 | -22.41 | 52.53 | 0.4486 | 825.0 | 759.9 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 22.29 | 214.20 | -22.53 | 51.31 | 0.4561 | 799.0 | 630.5 | |
| 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. | |