| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.57 | 119.12 | 19.01 | 115.99 | 18.95 | 105.15 | -57.77 | 68.40 | 0.8625 | -713.7 | -181.1 | |
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back to the solar disc SDO HMI 2011-12-01 05:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.86 | 22.77 | 104.75 | -58.17 | 64.17 | 0.8724 | -536.0 | -422.1 | |
| 18.89 | 117.76 | 18.34 | 114.57 | 18.92 | 105.19 | -57.73 | 68.43 | 0.8622 | -815.0 | -182.3 | |
| 0.68 | -2.00 | 0.67 | -2.00 | 18.94 | 104.76 | -58.16 | 68.49 | 0.8658 | 180.4 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.56 | 19.03 | 101.45 | -61.47 | 69.00 | 0.8916 | 368.0 | 401.8 | |
| 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. | |