SDO HMI 2014-03-08 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.93 | 0.00 | 10.81 | -16.26 | 44.84 | 13.81 | 234.89 | 0.2815 | 114.9 | -14.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.32 | -15.89 | 47.82 | 16.79 | 240.75 | 0.3199 | 709.0 | 460.4 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -17.10 | 46.92 | 15.90 | 236.11 | 0.3168 | -557.0 | -510.9 | |
| 0.00 | 2.16 | 0.00 | 1.12 | -16.06 | 46.54 | 15.52 | 238.48 | 0.3030 | 677.0 | 681.4 | |
| 0.00 | 2.08 | 0.00 | 1.08 | -15.70 | 46.42 | 15.40 | 239.35 | 0.2984 | 1082.0 | 963.8 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -15.53 | 46.15 | 15.13 | 239.46 | 0.2932 | 1005.0 | 855.9 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -15.77 | 46.07 | 15.05 | 238.60 | 0.2940 | 894.0 | 699.6 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -16.57 | 45.59 | 14.56 | 235.45 | 0.2940 | 914.0 | 695.4 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -19.78 | 45.67 | 14.64 | 227.10 | 0.3261 | 774.0 | 534.9 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -15.11 | 44.91 | 13.89 | 238.76 | 0.2722 | 810.0 | 710.3 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -16.77 | 43.59 | 12.57 | 231.03 | 0.2692 | -850.0 | -703.5 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -17.08 | 43.42 | 12.39 | 229.75 | 0.2701 | -1018.0 | -787.5 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -16.87 | 43.38 | 12.35 | 230.27 | 0.2673 | -921.0 | -734.7 | |
| 0.00 | 1.64 | 0.00 | 0.84 | -16.66 | 43.30 | 12.27 | 230.74 | 0.2642 | -1055.0 | -916.7 | |
| 0.00 | 3.72 | 0.00 | 1.90 | -15.29 | 42.74 | 11.72 | 233.95 | 0.2434 | -855.0 | -756.5 | |
| 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. | |