| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.01 | 109.73 | 17.27 | 111.93 | 19.09 | 105.17 | -59.39 | 68.58 | 0.8756 | -663.1 | -187.1 | |
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back to the solar disc SDO HMI 2011-12-01 02:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 1.15 | 28.89 | 101.42 | -63.14 | 58.61 | 0.9168 | -347.0 | -309.2 | |
| 0.00 | 1.03 | 0.00 | 0.97 | 19.85 | 108.07 | -56.49 | 67.11 | 0.8534 | 431.0 | 393.3 | |
| 0.00 | 1.11 | 0.00 | 1.26 | 25.29 | 102.95 | -61.61 | 62.15 | 0.9015 | -359.0 | -272.2 | |
| 17.01 | 106.65 | 17.27 | 108.55 | 18.91 | 105.21 | -59.35 | 68.77 | 0.8751 | -762.4 | -190.5 | |
| 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. | |