SDO HMI 2011-08-05 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.27 | 28.85 | 0.80 | 18.44 | 18.53 | 242.29 | -37.95 | 67.81 | 0.6313 | -12.9 | 49.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.83 | 19.40 | 246.46 | -33.78 | 64.72 | 0.5822 | -558.0 | -436.5 | |
| 0.00 | 2.35 | 0.00 | 1.43 | 18.27 | 246.37 | -33.87 | 66.64 | 0.5786 | -878.0 | -683.7 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 18.42 | 246.26 | -33.98 | 66.45 | 0.5807 | -741.0 | -642.4 | |
| 0.00 | 1.18 | 0.00 | 0.72 | 17.95 | 245.67 | -34.57 | 67.49 | 0.5866 | -649.0 | -601.5 | |
| 0.00 | 1.72 | 0.00 | 1.06 | 17.98 | 245.19 | -35.05 | 67.63 | 0.5929 | -812.0 | -672.6 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 18.03 | 244.91 | -35.34 | 67.67 | 0.5968 | -489.0 | -493.8 | |
| 1.27 | 6.24 | 0.80 | 3.95 | 18.13 | 242.97 | -37.27 | 68.25 | 0.6219 | -695.8 | -700.9 | |
| 0.00 | 3.44 | 0.00 | 2.25 | 18.94 | 240.41 | -39.83 | 67.89 | 0.6562 | 830.0 | 721.2 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 18.22 | 240.44 | -39.80 | 68.96 | 0.6537 | 844.0 | 757.3 | |
| 0.00 | 0.72 | 0.00 | 0.48 | 19.39 | 240.02 | -40.22 | 67.36 | 0.6622 | 555.0 | 490.0 | |
| 0.00 | 1.99 | 0.00 | 1.31 | 19.10 | 239.94 | -40.30 | 67.81 | 0.6624 | 660.0 | 575.6 | |
| 0.00 | 4.52 | 0.00 | 2.98 | 18.82 | 239.98 | -40.26 | 68.21 | 0.6611 | 864.0 | 657.8 | |
| 0.00 | 2.80 | 0.00 | 1.85 | 18.36 | 239.73 | -40.51 | 68.96 | 0.6628 | 766.0 | 611.0 | |
| 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. | |