SDO HMI 2014-10-04 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.55 | 30.22 | 1.32 | 15.91 | -12.73 | 139.60 | 3.24 | 189.70 | 0.3367 | 153.4 | 311.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 1.04 | -15.77 | 140.85 | 4.49 | 191.23 | 0.3884 | 720.0 | 604.3 | |
| 0.00 | 2.02 | 0.00 | 1.09 | -15.83 | 140.66 | 4.30 | 190.74 | 0.3888 | 805.0 | 676.1 | |
| 2.55 | 11.42 | 1.32 | 5.92 | -10.04 | 140.42 | 4.06 | 193.73 | 0.2948 | 1109.9 | 818.5 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -12.37 | 140.36 | 3.99 | 191.86 | 0.3323 | 827.0 | 646.0 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.77 | 140.38 | 4.02 | 190.08 | 0.3869 | 786.0 | 645.3 | |
| 0.00 | 2.37 | 0.00 | 1.24 | -11.64 | 139.95 | 3.58 | 191.11 | 0.3191 | 736.0 | 671.0 | |
| 0.00 | 2.02 | 0.00 | 1.08 | -15.37 | 139.28 | 2.92 | 187.51 | 0.3778 | -719.0 | -689.2 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -18.17 | 138.69 | 2.33 | 185.28 | 0.4216 | -95.0 | -147.3 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -15.49 | 138.35 | 1.99 | 185.10 | 0.3782 | -744.0 | -571.8 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -10.34 | 138.29 | 1.92 | 186.49 | 0.2935 | 816.0 | 635.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -14.94 | 138.04 | 1.67 | 184.41 | 0.3688 | -853.0 | -695.8 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -14.68 | 137.88 | 1.52 | 184.05 | 0.3645 | -893.0 | -769.5 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -10.77 | 134.02 | -2.35 | 172.30 | 0.3016 | -808.0 | -566.5 | |
| 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. | |