SDO HMI 2014-11-29 15:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.96 | 28.72 | 3.13 | 17.76 | 16.66 | 152.30 | 33.82 | 297.02 | 0.6006 | 76.7 | 76.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.68 | 7.18 | 2.35 | 4.59 | 17.20 | 154.75 | 36.28 | 296.43 | 0.6335 | 850.3 | 531.0 | |
| 0.00 | 2.56 | 0.00 | 1.59 | 15.47 | 153.06 | 34.58 | 294.70 | 0.6044 | 828.0 | 649.9 | |
| 0.00 | 3.42 | 0.00 | 2.11 | 15.47 | 152.69 | 34.21 | 294.90 | 0.5997 | 913.0 | 750.7 | |
| 0.00 | 1.37 | 0.00 | 0.84 | 15.45 | 152.31 | 33.84 | 295.07 | 0.5948 | 693.0 | 654.1 | |
| 0.00 | 0.68 | 0.00 | 0.42 | 16.76 | 152.31 | 33.83 | 297.14 | 0.6013 | 629.0 | 523.9 | |
| 0.00 | 1.28 | 0.00 | 0.79 | 16.55 | 152.19 | 33.72 | 296.87 | 0.5988 | 542.0 | 448.9 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 17.21 | 151.03 | 32.55 | 298.62 | 0.5878 | -681.0 | -533.7 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 17.06 | 150.89 | 32.41 | 298.47 | 0.5852 | -594.0 | -510.5 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 15.80 | 150.61 | 32.14 | 296.64 | 0.5749 | -587.0 | -468.3 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 17.46 | 150.75 | 32.27 | 299.20 | 0.5857 | -644.0 | -456.9 | |
| 1.28 | 2.74 | 0.78 | 1.65 | 16.54 | 150.35 | 31.88 | 298.00 | 0.5755 | -832.1 | -671.8 | |
| 0.00 | 4.02 | 0.00 | 2.44 | 17.28 | 150.35 | 31.87 | 299.18 | 0.5797 | -739.0 | -655.3 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 17.77 | 150.37 | 31.90 | 299.94 | 0.5829 | -625.0 | -498.8 | |
| 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. | |