| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.54 | 85.74 | 69.21 | 456.27 | -22.70 | 106.44 | 84.08 | 247.23 | 0.9956 | 387.3 | 271.9 | |
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back to the solar disc SDO HMI 2011-12-11 21:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.81 | 17.97 | 34.63 | 92.14 | -21.29 | 106.33 | 83.98 | 248.65 | 0.9954 | 531.2 | 412.1 | |
| 1.79 | 66.07 | 10.46 | 358.07 | -23.10 | 107.41 | 85.05 | 246.85 | 0.9970 | -190.6 | 244.2 | |
| 4.94 | -2.00 | 24.12 | -2.00 | -23.05 | 106.12 | 83.76 | 246.87 | 0.9952 | 430.0 | 999999 | |
| 0.00 | 1.70 | 0.00 | 6.06 | -22.67 | 103.83 | 81.47 | 247.16 | 0.9908 | 420.0 | 422.1 | |
| 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. | |