SDO HMI 2011-08-28 09:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.34 | 233.05 | 23.60 | 156.40 | 13.41 | 291.40 | -42.64 | 77.86 | 0.6761 | -472.6 | -222.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.88 | 215.47 | 19.25 | 144.03 | 13.44 | 291.81 | -42.23 | 77.78 | 0.6711 | -1017.7 | -296.8 | |
| 1.88 | -1.00 | 1.27 | -1.00 | 13.52 | 291.24 | -42.79 | 77.73 | 0.6783 | -550.3 | 999999 | |
| 3.86 | -1.00 | 2.60 | -1.00 | 13.38 | 291.02 | -43.02 | 77.96 | 0.6810 | -499.9 | 999999 | |
| 0.72 | -1.00 | 0.48 | -1.00 | 13.11 | 291.08 | -42.96 | 78.35 | 0.6800 | -376.6 | 999999 | |
| 0.00 | 1.52 | 0.00 | 1.05 | 12.00 | 289.90 | -44.14 | 80.06 | 0.6939 | 622.0 | 539.4 | |
| 0.00 | 1.08 | 0.00 | 0.74 | 12.24 | 289.54 | -44.50 | 79.73 | 0.6984 | 617.0 | 495.3 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 13.80 | 289.05 | -44.99 | 77.54 | 0.7054 | 579.0 | 387.3 | |
| 0.00 | 1.70 | 0.00 | 1.19 | 13.70 | 288.67 | -45.36 | 77.71 | 0.7098 | 657.0 | 575.1 | |
| 0.00 | 2.51 | 0.00 | 1.77 | 13.59 | 288.48 | -45.56 | 77.88 | 0.7121 | 646.0 | 559.5 | |
| 0.00 | 3.59 | 0.00 | 2.52 | 13.16 | 288.45 | -45.59 | 78.49 | 0.7121 | 571.0 | 539.3 | |
| 0.00 | 0.90 | 0.00 | 0.63 | 13.31 | 288.10 | -45.94 | 78.30 | 0.7164 | 495.0 | 409.0 | |
| 0.00 | 1.52 | 0.00 | 1.08 | 13.52 | 287.96 | -46.08 | 78.03 | 0.7182 | 490.0 | 347.9 | |
| 0.00 | 2.96 | 0.00 | 2.13 | 14.04 | 287.19 | -46.85 | 77.37 | 0.7276 | 593.0 | 510.4 | |
| 0.00 | 0.90 | 0.00 | 0.64 | 11.78 | 287.38 | -46.66 | 80.48 | 0.7243 | 523.0 | 387.4 | |
| 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. | |