SDO HMI 2011-10-29 08:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.87 | 102.66 | 35.65 | 115.55 | 12.82 | 300.49 | 64.16 | 282.02 | 0.8981 | 263.6 | 68.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.21 | 4.94 | 4.66 | 7.17 | 12.84 | 306.85 | 70.53 | 281.98 | 0.9412 | -456.3 | -362.9 | |
| 1.65 | 2.78 | 2.38 | 4.02 | 13.15 | 306.87 | 70.55 | 282.31 | 0.9413 | -323.3 | -273.5 | |
| 0.87 | 2.25 | 1.19 | 3.09 | 12.84 | 305.68 | 69.36 | 281.97 | 0.9342 | -308.0 | -367.5 | |
| 2.25 | 6.24 | 2.82 | 7.82 | 11.43 | 303.41 | 67.09 | 280.44 | 0.9198 | -478.4 | -375.1 | |
| 3.38 | 4.25 | 3.97 | 4.99 | 11.94 | 301.75 | 65.42 | 281.01 | 0.9082 | 355.9 | 305.9 | |
| 0.00 | 0.95 | 0.00 | 1.11 | 13.60 | 301.61 | 65.29 | 282.84 | 0.9074 | 41.0 | 37.3 | |
| 0.00 | 10.06 | 0.00 | 11.64 | 13.34 | 301.33 | 65.01 | 282.57 | 0.9053 | -193.0 | -54.0 | |
| 0.00 | 1.21 | 0.00 | 1.40 | 13.60 | 301.24 | 64.92 | 282.84 | 0.9047 | 402.0 | 375.6 | |
| 0.00 | 1.30 | 0.00 | 1.44 | 13.07 | 300.05 | 63.73 | 282.29 | 0.8958 | -411.0 | -308.2 | |
| 0.00 | 0.78 | 0.00 | 0.85 | 13.60 | 299.47 | 63.15 | 282.90 | 0.8915 | 233.0 | 184.9 | |
| 19.51 | 65.30 | 20.63 | 69.28 | 12.86 | 298.73 | 62.40 | 282.09 | 0.8855 | 638.4 | 165.2 | |
| 0.00 | 1.39 | 0.00 | 1.47 | 13.65 | 298.75 | 62.43 | 282.98 | 0.8859 | 458.0 | 412.9 | |
| 0.00 | 1.21 | 0.00 | 1.27 | 13.34 | 298.41 | 62.09 | 282.64 | 0.8831 | 740.0 | 621.1 | |
| 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. | |