| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.27 | 259.70 | 29.22 | 215.25 | 27.69 | 45.73 | -49.92 | 57.72 | 0.8037 | -968.1 | -305.3 | |
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back to the solar disc SDO HMI 2011-11-09 00:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.49 | 258.15 | 28.57 | 213.91 | 27.69 | 45.76 | -49.89 | 57.71 | 0.8035 | -1026.3 | -305.4 | |
| 0.78 | -1.00 | 0.65 | -1.00 | 27.53 | 45.13 | -50.53 | 58.11 | 0.8085 | -306.9 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.97 | 27.52 | 43.62 | -52.03 | 58.58 | 0.8215 | -274.0 | -249.9 | |
| 0.00 | 0.43 | 0.00 | 0.37 | 27.54 | 43.34 | -52.32 | 58.65 | 0.8240 | -429.0 | -422.0 | |
| 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. | |