| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.06 | 56.14 | 12.23 | 76.19 | 15.93 | 232.90 | 67.79 | 286.79 | 0.9316 | -432.5 | -8.3 | |
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back to the solar disc SDO HMI 2011-12-01 01:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.06 | 48.36 | 12.23 | 65.82 | 15.54 | 232.98 | 67.87 | 286.36 | 0.9318 | -611.9 | -41.9 | |
| 0.00 | 1.54 | 0.00 | 1.95 | 16.61 | 231.40 | 66.29 | 287.68 | 0.9225 | -355.0 | -349.1 | |
| 0.00 | 1.71 | 0.00 | 2.17 | 16.92 | 231.38 | 66.27 | 288.01 | 0.9227 | -295.0 | -252.4 | |
| 0.00 | 0.94 | 0.00 | 1.29 | 19.24 | 232.94 | 67.83 | 290.31 | 0.9339 | 498.0 | 435.5 | |
| 0.00 | 3.59 | 0.00 | 4.96 | 19.61 | 233.10 | 67.99 | 290.69 | 0.9351 | 616.0 | 480.1 | |
| 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. | |