| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 32.07 | 0.00 | 226.30 | -17.17 | 107.35 | 84.73 | 252.51 | 0.9967 | -175.2 | -9.5 | |
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back to the solar disc SDO HMI 2011-11-14 13:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.00 | 0.00 | 91.62 | -16.45 | 108.11 | 85.49 | 253.31 | 0.9984 | 68.0 | 78.7 | |
| 0.00 | 6.28 | 0.00 | 54.83 | -17.29 | 108.21 | 85.59 | 252.47 | 0.9986 | -215.0 | -117.9 | |
| 0.00 | 7.14 | 0.00 | 63.33 | -18.13 | 108.01 | 85.39 | 251.62 | 0.9985 | -8.0 | 6.7 | |
| 0.00 | 5.59 | 0.00 | 12.30 | -17.08 | 98.07 | 75.45 | 251.72 | 0.9754 | -311.0 | -138.5 | |
| 0.00 | 2.06 | 0.00 | 4.22 | -17.24 | 96.93 | 74.30 | 251.41 | 0.9712 | -410.0 | -384.5 | |
| 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. | |