SDO HMI 2011-08-10 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.12 | 0.00 | 12.96 | 19.31 | 224.02 | 9.34 | 326.23 | 0.2751 | -332.4 | -361.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.35 | 0.00 | 1.22 | 20.02 | 226.63 | 11.95 | 320.77 | 0.3089 | -988.0 | -776.3 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 20.36 | 226.59 | 11.91 | 321.60 | 0.3128 | -695.0 | -552.4 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 20.31 | 226.09 | 11.41 | 322.64 | 0.3071 | -799.0 | -691.3 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 19.56 | 226.03 | 11.35 | 321.14 | 0.2970 | -837.0 | -660.0 | |
| 0.00 | 4.70 | 0.00 | 2.44 | 20.01 | 225.47 | 10.79 | 323.49 | 0.2971 | -708.0 | -746.5 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.04 | 224.33 | 9.66 | 321.94 | 0.2599 | -908.0 | -733.1 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 17.55 | 224.08 | 9.40 | 321.41 | 0.2509 | -876.0 | -736.9 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 20.23 | 224.07 | 9.39 | 327.55 | 0.2867 | -762.0 | -612.1 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 17.89 | 223.78 | 9.10 | 323.19 | 0.2523 | -692.0 | -582.4 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 18.70 | 223.62 | 8.95 | 325.57 | 0.2617 | -1091.0 | -940.3 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 19.32 | 221.93 | 7.26 | 332.08 | 0.2557 | 891.0 | 701.4 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 18.89 | 221.46 | 6.79 | 332.80 | 0.2457 | 782.0 | 665.6 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.20 | 221.35 | 6.67 | 333.80 | 0.2495 | 1157.0 | 814.5 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 19.30 | 218.31 | 3.63 | 345.04 | 0.2328 | 873.0 | 584.5 | |
| 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. | |