SDO HMI 2014-09-09 05:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.72 | 41.73 | 8.32 | 25.13 | 9.55 | 147.28 | 34.89 | 276.34 | 0.5693 | -49.3 | -84.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.10 | 11.77 | 2.57 | 7.36 | 9.41 | 150.35 | 37.96 | 276.02 | 0.6125 | -753.0 | -612.9 | |
| 1.78 | -1.00 | 1.11 | -1.00 | 9.66 | 150.27 | 37.88 | 276.43 | 0.6114 | -762.8 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.55 | 9.50 | 149.94 | 37.55 | 276.17 | 0.6068 | -617.0 | -586.7 | |
| 0.62 | 4.64 | 0.38 | 2.79 | 9.95 | 147.25 | 34.86 | 277.01 | 0.5695 | -916.7 | -734.2 | |
| 0.45 | 1.25 | 0.27 | 0.75 | 9.04 | 147.14 | 34.76 | 275.42 | 0.5677 | -576.0 | -466.7 | |
| 0.00 | 1.52 | 0.00 | 0.91 | 10.16 | 147.24 | 34.85 | 277.39 | 0.5694 | -782.0 | -648.4 | |
| 0.00 | 2.05 | 0.00 | 1.23 | 8.92 | 146.72 | 34.34 | 275.21 | 0.5617 | -918.0 | -750.3 | |
| 0.62 | 8.38 | 0.37 | 4.94 | 9.33 | 145.70 | 33.31 | 275.97 | 0.5470 | 675.3 | 624.7 | |
| 0.00 | 1.69 | 0.00 | 1.00 | 9.98 | 145.55 | 33.16 | 277.16 | 0.5451 | 587.0 | 524.8 | |
| 4.10 | -8.00 | 2.42 | -8.00 | 9.47 | 145.42 | 33.03 | 276.24 | 0.5430 | 919.4 | 999999 | |
| 2.05 | 5.98 | 1.20 | 3.51 | 9.82 | 145.13 | 32.74 | 276.91 | 0.5389 | 865.4 | 676.5 | |
| 0.00 | 0.71 | 0.00 | 0.42 | 9.04 | 144.97 | 32.59 | 275.46 | 0.5364 | 604.0 | 528.0 | |
| 0.00 | 2.85 | 0.00 | 1.67 | 9.23 | 144.88 | 32.50 | 275.82 | 0.5351 | 863.0 | 611.3 | |
| 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. | |