| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.21 | 39.29 | 8.06 | 22.20 | -20.19 | 249.22 | -12.53 | 155.01 | 0.4829 | 629.7 | 391.3 | |
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back to the solar disc SDO HMI 2014-08-01 16:00:39 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.53 | 0.00 | 1.39 | -17.09 | 251.39 | -10.35 | 156.08 | 0.4255 | -825.0 | -643.5 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -18.32 | 251.12 | -10.62 | 156.73 | 0.4449 | 912.0 | 834.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -17.36 | 251.15 | -10.60 | 155.86 | 0.4310 | -628.0 | -476.8 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -18.06 | 250.97 | -10.77 | 156.20 | 0.4421 | 734.0 | 564.9 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -17.59 | 250.94 | -10.81 | 155.67 | 0.4357 | 764.0 | 615.1 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -22.60 | 249.09 | -12.65 | 156.87 | 0.5169 | 190.0 | 281.4 | |
| 14.21 | 24.43 | 8.06 | 13.85 | -20.48 | 249.02 | -12.73 | 154.89 | 0.4884 | 974.0 | 614.1 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -22.96 | 248.79 | -12.96 | 156.67 | 0.5235 | 717.0 | 583.8 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -19.03 | 248.94 | -12.81 | 153.35 | 0.4692 | 726.0 | 606.9 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.07 | 248.77 | -12.98 | 153.09 | 0.4709 | 576.0 | 457.9 | |
| 0.00 | 0.36 | 0.00 | 0.20 | -19.20 | 247.70 | -14.05 | 151.36 | 0.4802 | 608.0 | 452.0 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.20 | 247.40 | -14.35 | 150.86 | 0.4825 | 720.0 | 579.1 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -24.82 | 246.03 | -15.72 | 154.08 | 0.5646 | 288.0 | 286.1 | |
| 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. | |