SDO HMI 2014-10-11 20:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.22 | 0.00 | 9.47 | 13.40 | 57.65 | 15.85 | 297.50 | 0.3003 | 273.9 | 248.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.43 | 11.92 | 66.98 | 25.18 | 284.93 | 0.4327 | -691.0 | -605.6 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 13.44 | 66.06 | 24.26 | 288.87 | 0.4241 | -566.0 | -538.3 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 8.41 | 62.77 | 20.97 | 277.54 | 0.3587 | -818.0 | -593.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 18.22 | 60.77 | 18.98 | 304.84 | 0.3780 | -783.0 | -689.0 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 12.72 | 59.70 | 17.90 | 291.81 | 0.3244 | 802.0 | 699.7 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 15.58 | 59.22 | 17.42 | 300.38 | 0.3358 | -850.0 | -687.4 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 14.15 | 55.48 | 13.68 | 301.86 | 0.2713 | 668.0 | 469.1 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 13.57 | 55.41 | 13.62 | 300.09 | 0.2657 | 821.0 | 705.7 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 13.79 | 55.33 | 13.53 | 300.94 | 0.2662 | 756.0 | 635.1 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 13.06 | 55.26 | 13.46 | 298.62 | 0.2595 | 908.0 | 689.1 | |
| 0.00 | 0.44 | 0.00 | 0.22 | 13.35 | 54.58 | 12.78 | 300.82 | 0.2518 | 825.0 | 643.6 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 11.09 | 53.47 | 11.67 | 294.10 | 0.2185 | 913.0 | 759.7 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 14.52 | 52.28 | 10.48 | 310.00 | 0.2310 | 921.0 | 761.9 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 14.56 | 51.75 | 9.95 | 311.57 | 0.2246 | 928.0 | 677.8 | |
| 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. | |