SDO HMI 2014-10-03 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 |
| 7.73 | 31.41 | 4.05 | 16.59 | -10.80 | 139.33 | -10.22 | 149.71 | 0.3464 | 64.7 | 272.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.92 | 14.51 | 2.58 | 7.60 | -9.95 | 140.33 | -9.22 | 150.87 | 0.3257 | 1131.1 | 794.0 | |
| 1.49 | 4.40 | 0.78 | 2.30 | -9.33 | 140.20 | -9.36 | 149.53 | 0.3179 | 1079.5 | 866.7 | |
| 1.32 | -1.00 | 0.69 | -1.00 | -9.80 | 140.15 | -9.40 | 150.16 | 0.3250 | 1084.3 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -11.69 | 139.87 | -9.68 | 152.17 | 0.3544 | 798.0 | 664.6 | |
| 0.00 | 1.76 | 0.00 | 0.94 | -12.42 | 139.66 | -9.90 | 152.62 | 0.3666 | 926.0 | 765.9 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -11.18 | 139.71 | -9.85 | 151.07 | 0.3485 | 738.0 | 583.5 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -13.64 | 138.82 | -10.73 | 152.25 | 0.3904 | -808.0 | -590.9 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -13.18 | 138.34 | -11.21 | 150.61 | 0.3874 | -858.0 | -721.6 | |
| 0.00 | 2.11 | 0.00 | 1.13 | -13.02 | 138.10 | -11.46 | 149.87 | 0.3872 | -667.0 | -557.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -14.60 | 137.73 | -11.82 | 151.10 | 0.4120 | -851.0 | -641.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -12.74 | 137.83 | -11.73 | 148.91 | 0.3856 | -763.0 | -613.6 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -11.07 | 136.56 | -13.00 | 143.70 | 0.3744 | -837.0 | -652.8 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -10.80 | 133.70 | -15.85 | 137.68 | 0.4003 | -468.0 | -481.0 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -10.59 | 133.56 | -16.00 | 137.05 | 0.3993 | -745.0 | -634.6 | |
| 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. | |