SDO HMI 2014-01-16 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.07 | 333.16 | 37.64 | 190.05 | -16.22 | 12.15 | 27.87 | 245.01 | 0.4972 | 951.6 | 389.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.83 | -17.11 | 18.16 | 33.88 | 246.80 | 0.5819 | 618.0 | 477.2 | |
| 26.53 | 191.31 | 15.25 | 110.05 | -16.53 | 12.93 | 28.64 | 244.95 | 0.5093 | 1133.0 | 357.9 | |
| 8.08 | -2.00 | 4.63 | -2.00 | -16.60 | 12.59 | 28.30 | 244.59 | 0.5051 | 1243.3 | 999999 | |
| 0.00 | 5.70 | 0.00 | 3.23 | -15.20 | 12.03 | 27.75 | 246.90 | 0.4904 | 121.0 | -7.7 | |
| 0.00 | 2.81 | 0.00 | 1.59 | -16.55 | 11.50 | 27.22 | 243.95 | 0.4900 | 586.0 | 569.5 | |
| 31.46 | 121.25 | 17.76 | 68.38 | -15.68 | 11.27 | 26.99 | 245.47 | 0.4822 | 1220.8 | 494.1 | |
| 0.00 | 3.91 | 0.00 | 2.20 | -14.79 | 11.15 | 26.86 | 247.17 | 0.4760 | 1012.0 | 862.8 | |
| 0.00 | 1.96 | 0.00 | 1.10 | -14.32 | 10.81 | 26.53 | 247.91 | 0.4690 | -623.0 | -502.7 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -18.95 | 11.44 | 27.16 | 239.44 | 0.5034 | 657.0 | 541.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -19.74 | 10.60 | 26.32 | 237.31 | 0.4978 | 657.0 | 498.7 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -19.01 | 4.43 | 20.14 | 232.24 | 0.4136 | -714.0 | -615.0 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -18.35 | 4.25 | 19.96 | 233.38 | 0.4055 | -797.0 | -628.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -19.61 | 1.01 | 16.72 | 226.10 | 0.3778 | -898.0 | -721.0 | |
| 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. | |