| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.29 | 172.77 | 15.38 | 90.73 | 17.92 | 299.91 | -16.51 | 54.64 | 0.3329 | -1206.1 | -422.9 | |
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back to the solar disc SDO HMI 2011-08-29 17:59:08 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.79 | 0.00 | 0.92 | 14.06 | 302.00 | -14.41 | 62.75 | 0.2728 | -946.0 | -683.7 | |
| 0.00 | 1.34 | 0.00 | 0.69 | 13.99 | 301.52 | -14.89 | 63.69 | 0.2795 | -842.0 | -660.7 | |
| 29.29 | 169.01 | 15.38 | 88.78 | 17.98 | 299.89 | -16.53 | 54.49 | 0.3338 | -1282.8 | -417.1 | |
| 0.00 | 0.63 | 0.00 | 0.34 | 19.34 | 297.29 | -19.12 | 54.82 | 0.3798 | -650.0 | -474.6 | |
| 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. | |