SDO HMI 2011-11-28 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.98 | 229.98 | 28.21 | 143.91 | 15.63 | 233.38 | 35.29 | 294.40 | 0.6132 | -964.7 | -348.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.84 | 18.28 | 235.51 | 37.42 | 297.26 | 0.6514 | -619.0 | -435.8 | |
| 3.25 | 3.85 | 2.10 | 2.49 | 17.76 | 235.26 | 37.17 | 296.63 | 0.6460 | -630.2 | -559.7 | |
| 0.00 | 1.20 | 0.00 | 0.77 | 17.92 | 234.76 | 36.67 | 297.13 | 0.6407 | -642.0 | -522.6 | |
| 35.31 | 213.13 | 22.10 | 133.36 | 15.42 | 233.48 | 35.39 | 294.01 | 0.6135 | -1152.5 | -335.8 | |
| 0.00 | 1.62 | 0.00 | 1.00 | 13.27 | 232.72 | 34.63 | 290.97 | 0.5946 | -368.0 | -329.5 | |
| 2.91 | -4.00 | 1.82 | -4.00 | 16.22 | 233.19 | 35.10 | 295.40 | 0.6135 | -863.1 | 999999 | |
| 3.51 | -4.00 | 2.19 | -4.00 | 15.91 | 233.05 | 34.96 | 295.00 | 0.6103 | -918.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.84 | 13.54 | 232.47 | 34.38 | 291.54 | 0.5925 | -761.0 | -517.4 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 18.20 | 231.99 | 33.91 | 299.12 | 0.6089 | -678.0 | -460.6 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 18.73 | 231.92 | 33.84 | 299.96 | 0.6110 | -637.0 | -521.7 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 17.04 | 230.71 | 32.62 | 298.13 | 0.5867 | -738.0 | -606.0 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 17.73 | 230.04 | 31.95 | 299.65 | 0.5822 | -673.0 | -519.5 | |
| 0.00 | 2.74 | 0.00 | 1.66 | 17.92 | 229.97 | 31.88 | 299.99 | 0.5824 | -681.0 | -626.8 | |
| 0.00 | 0.51 | 0.00 | 0.31 | 18.16 | 229.94 | 31.86 | 300.39 | 0.5836 | -687.0 | -514.2 | |
| 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. | |