SDO HMI 2014-10-11 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.38 | 0.00 | 9.42 | 14.03 | 57.81 | 11.61 | 308.26 | 0.2448 | 22.8 | 104.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.70 | 11.97 | 66.81 | 20.61 | 287.49 | 0.3626 | -789.0 | -618.5 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 12.62 | 62.76 | 16.55 | 292.91 | 0.3031 | -827.0 | -633.8 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 17.93 | 60.56 | 14.35 | 311.40 | 0.3157 | -822.0 | -613.6 | |
| 0.00 | 2.63 | 0.00 | 1.35 | 12.82 | 60.03 | 13.83 | 297.17 | 0.2631 | 814.0 | 642.4 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 17.75 | 60.38 | 14.17 | 311.28 | 0.3117 | -902.0 | -755.8 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 12.46 | 59.95 | 13.74 | 296.04 | 0.2594 | 672.0 | 515.6 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 16.89 | 59.70 | 13.49 | 310.34 | 0.2942 | -757.0 | -591.6 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 15.59 | 59.22 | 13.02 | 307.61 | 0.2751 | -730.0 | -518.2 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 16.41 | 59.12 | 12.91 | 310.22 | 0.2820 | -750.0 | -575.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 13.49 | 55.55 | 9.34 | 309.39 | 0.2052 | 761.0 | 657.9 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 13.62 | 52.91 | 6.71 | 319.15 | 0.1743 | 815.0 | 679.8 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 14.38 | 52.19 | 5.98 | 325.02 | 0.1769 | 823.0 | 722.6 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 11.45 | 50.74 | 4.53 | 320.27 | 0.1217 | 1028.0 | 815.8 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 11.63 | 50.56 | 4.35 | 322.35 | 0.1222 | 983.0 | 750.6 | |
| 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. | |