| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.69 | 98.22 | 17.09 | 114.52 | 18.87 | 105.36 | -63.61 | 69.54 | 0.9065 | -622.6 | -167.0 | |
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back to the solar disc SDO HMI 2011-11-30 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 1.29 | 20.44 | 105.51 | -63.46 | 67.80 | 0.9072 | -415.0 | -336.5 | |
| 0.00 | 0.94 | 0.00 | 1.10 | 20.60 | 105.33 | -63.65 | 67.66 | 0.9086 | -530.0 | -466.9 | |
| 13.49 | 96.17 | 15.68 | 112.13 | 18.84 | 105.39 | -63.58 | 69.57 | 0.9063 | -712.3 | -161.3 | |
| 1.20 | -3.00 | 1.41 | -3.00 | 18.74 | 105.03 | -63.94 | 69.73 | 0.9086 | 161.3 | 999999 | |
| 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. | |