| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.92 | 140.85 | 16.97 | 96.00 | 17.63 | 300.19 | -43.20 | 71.76 | 0.6892 | -937.6 | -320.8 | |
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back to the solar disc SDO HMI 2011-08-27 16:59:08 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.92 | 136.90 | 16.97 | 93.21 | 17.68 | 300.26 | -43.13 | 71.68 | 0.6884 | -1010.4 | -316.0 | |
| 0.00 | 0.45 | 0.00 | 0.32 | 16.19 | 298.00 | -45.39 | 74.20 | 0.7128 | -636.0 | -567.0 | |
| 0.00 | 2.87 | 0.00 | 2.03 | 16.01 | 297.78 | -45.61 | 74.48 | 0.7152 | -519.0 | -438.3 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 16.34 | 297.64 | -45.75 | 74.04 | 0.7173 | -423.0 | -425.4 | |
| 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. | |