SDO HMI 2011-08-10 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.38 | 0.00 | 11.57 | 19.03 | 223.37 | 10.34 | 322.85 | 0.2805 | -108.5 | -182.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.57 | 20.01 | 226.67 | 13.64 | 317.14 | 0.3272 | -854.0 | -699.6 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 20.31 | 226.17 | 13.13 | 318.82 | 0.3250 | -747.0 | -689.7 | |
| 0.00 | 4.34 | 0.00 | 2.26 | 20.07 | 225.38 | 12.35 | 319.99 | 0.3138 | -769.0 | -788.3 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 17.82 | 224.20 | 11.17 | 317.41 | 0.2737 | -898.0 | -712.1 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 18.04 | 224.12 | 11.09 | 318.18 | 0.2754 | -901.0 | -747.6 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.08 | 223.83 | 10.79 | 319.00 | 0.2726 | -851.0 | -657.2 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 20.07 | 223.93 | 10.89 | 323.37 | 0.2988 | -886.0 | -730.5 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 18.71 | 223.67 | 10.64 | 320.93 | 0.2787 | -1010.0 | -805.0 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 19.39 | 221.85 | 8.82 | 327.45 | 0.2700 | 914.0 | 673.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 18.68 | 221.62 | 8.59 | 326.58 | 0.2580 | 845.0 | 618.4 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 19.06 | 221.51 | 8.48 | 327.74 | 0.2622 | 827.0 | 610.2 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 19.21 | 221.32 | 8.29 | 328.64 | 0.2628 | 934.0 | 611.9 | |
| 0.00 | 2.62 | 0.00 | 1.34 | 18.10 | 220.62 | 7.59 | 328.43 | 0.2408 | 872.0 | 738.3 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.20 | 220.34 | 7.30 | 329.61 | 0.2397 | 1005.0 | 792.7 | |
| 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. | |