| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.03 | 21.52 | 12.12 | 38.29 | -16.98 | 340.75 | 72.39 | 251.70 | 0.9613 | 304.7 | -119.5 | |
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back to the solar disc SDO HMI 2011-11-23 05:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 7.89 | 1.62 | 15.06 | -16.74 | 341.85 | 73.49 | 252.08 | 0.9661 | 270.5 | -368.7 | |
| 0.00 | 0.69 | 0.00 | 1.32 | -17.00 | 342.12 | 73.76 | 251.84 | 0.9674 | 92.0 | 42.9 | |
| 4.80 | 7.03 | 8.25 | 12.08 | -16.63 | 340.25 | 71.89 | 252.00 | 0.9589 | 496.6 | 351.8 | |
| 0.00 | 2.31 | 0.00 | 3.94 | -16.84 | 340.05 | 71.69 | 251.76 | 0.9580 | 386.0 | 358.7 | |
| 1.37 | 3.60 | 2.25 | 5.89 | -18.37 | 339.15 | 70.79 | 250.04 | 0.9548 | -315.8 | -271.5 | |
| 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. | |