SDO HMI 2014-07-22 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.56 | 169.64 | 20.83 | 105.69 | -20.99 | 68.96 | 27.24 | 224.86 | 0.6080 | 408.2 | 241.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.86 | 130.45 | 14.32 | 81.75 | -20.91 | 69.70 | 27.98 | 225.75 | 0.6142 | 1006.0 | 309.9 | |
| 0.54 | 14.24 | 0.34 | 8.82 | -20.79 | 68.43 | 26.71 | 224.61 | 0.6005 | 937.0 | 487.0 | |
| 2.27 | -2.00 | 1.41 | -2.00 | -21.02 | 68.44 | 26.72 | 224.33 | 0.6028 | 631.5 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -20.50 | 68.12 | 26.40 | 224.65 | 0.5949 | 788.0 | 660.4 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -19.42 | 67.92 | 26.21 | 225.83 | 0.5829 | 628.0 | 496.6 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -19.84 | 67.56 | 25.85 | 224.90 | 0.5832 | 742.0 | 693.6 | |
| 0.00 | 1.72 | 0.00 | 1.05 | -21.90 | 65.88 | 24.16 | 220.48 | 0.5872 | -618.0 | -505.4 | |
| 1.36 | 2.54 | 0.82 | 1.54 | -21.31 | 65.45 | 23.73 | 220.70 | 0.5772 | -808.1 | -643.9 | |
| 0.00 | 1.18 | 0.00 | 0.72 | -21.55 | 65.46 | 23.74 | 220.42 | 0.5797 | -742.0 | -484.7 | |
| 0.00 | 1.45 | 0.00 | 0.88 | -21.91 | 65.20 | 23.48 | 219.68 | 0.5811 | -704.0 | -481.4 | |
| 5.08 | 10.89 | 3.07 | 6.58 | -21.73 | 64.81 | 23.09 | 219.44 | 0.5756 | -916.3 | -750.0 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -21.25 | 63.95 | 22.23 | 218.97 | 0.5628 | -697.0 | -543.9 | |
| 1.45 | 2.90 | 0.87 | 1.75 | -22.10 | 63.87 | 22.16 | 217.88 | 0.5713 | -810.3 | -652.1 | |
| 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. | |