SDO HMI 2011-12-11 03:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.39 | 248.02 | 27.28 | 152.65 | 9.24 | 356.98 | -35.25 | 73.76 | 0.5955 | -662.1 | -243.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.95 | 201.42 | 19.50 | 123.05 | 9.41 | 357.69 | -34.54 | 73.22 | 0.5865 | -1166.6 | -413.1 | |
| 4.77 | -1.00 | 2.93 | -1.00 | 9.00 | 357.12 | -35.12 | 74.14 | 0.5929 | -770.0 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 7.83 | 357.02 | -35.22 | 76.10 | 0.5908 | 608.0 | 581.1 | |
| 0.00 | 2.73 | 0.00 | 1.68 | 8.10 | 356.63 | -35.61 | 75.79 | 0.5969 | -326.0 | -308.9 | |
| 0.00 | 1.19 | 0.00 | 0.74 | 7.92 | 356.50 | -35.74 | 76.12 | 0.5982 | -546.0 | -413.6 | |
| 1.79 | 2.64 | 1.11 | 1.64 | 8.82 | 356.33 | -35.91 | 74.71 | 0.6031 | -557.6 | -342.2 | |
| 0.00 | 1.19 | 0.00 | 0.75 | 9.87 | 355.46 | -36.78 | 73.35 | 0.6180 | 638.0 | 506.8 | |
| 2.81 | 5.37 | 1.77 | 3.37 | 8.82 | 355.32 | -36.91 | 75.06 | 0.6166 | -705.1 | -488.9 | |
| 0.00 | 0.68 | 0.00 | 0.43 | 8.58 | 355.24 | -37.00 | 75.47 | 0.6170 | -589.0 | -511.8 | |
| 1.79 | 26.75 | 1.15 | 17.06 | 8.86 | 353.88 | -38.35 | 75.47 | 0.6357 | 867.1 | 671.7 | |
| 1.28 | 1.79 | 0.82 | 1.15 | 8.62 | 353.49 | -38.75 | 75.95 | 0.6402 | 722.1 | 736.0 | |
| 0.00 | 1.19 | 0.00 | 0.77 | 8.08 | 353.44 | -38.80 | 76.80 | 0.6395 | 579.0 | 512.4 | |
| 0.00 | 0.68 | 0.00 | 0.44 | 8.57 | 352.41 | -39.82 | 76.35 | 0.6540 | 618.0 | 518.8 | |
| 0.00 | 1.79 | 0.00 | 1.20 | 8.19 | 350.64 | -41.59 | 77.38 | 0.6757 | 940.0 | 721.7 | |
| 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. | |