SDO HMI 2014-08-06 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.50 | 186.21 | 58.72 | 208.60 | 11.43 | 127.42 | -64.32 | 80.25 | 0.8976 | -129.6 | -3.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.89 | 102.19 | 34.63 | 107.79 | 12.50 | 129.18 | -62.56 | 79.10 | 0.8843 | -695.0 | -148.8 | |
| 0.00 | 4.43 | 0.00 | 4.74 | 11.50 | 128.71 | -63.04 | 80.23 | 0.8882 | -354.0 | -164.8 | |
| 0.00 | 1.72 | 0.00 | 1.88 | 12.55 | 127.98 | -63.77 | 79.04 | 0.8937 | 436.0 | 357.4 | |
| 0.00 | 2.26 | 0.00 | 2.41 | 10.21 | 128.78 | -62.97 | 81.69 | 0.8878 | 630.0 | 431.8 | |
| 0.00 | 1.17 | 0.00 | 1.28 | 11.81 | 128.09 | -63.66 | 79.87 | 0.8929 | 453.0 | 433.3 | |
| 0.00 | 1.08 | 0.00 | 1.17 | 11.03 | 128.34 | -63.41 | 80.75 | 0.8911 | -116.0 | -103.5 | |
| 0.00 | 1.45 | 0.00 | 1.58 | 10.88 | 128.04 | -63.70 | 80.91 | 0.8934 | -314.0 | -198.6 | |
| 0.00 | 4.97 | 0.00 | 5.55 | 9.65 | 127.43 | -64.31 | 82.27 | 0.8984 | 658.0 | 556.5 | |
| 0.00 | 0.81 | 0.00 | 0.94 | 10.99 | 126.62 | -65.12 | 80.75 | 0.9041 | 267.0 | 248.8 | |
| 0.00 | 0.90 | 0.00 | 1.04 | 10.06 | 126.55 | -65.20 | 81.78 | 0.9049 | 474.0 | 499.9 | |
| 0.00 | 2.98 | 0.00 | 3.44 | 9.77 | 126.51 | -65.24 | 82.09 | 0.9052 | 686.0 | 580.1 | |
| 0.90 | 2.26 | 1.05 | 2.63 | 10.39 | 126.19 | -65.55 | 81.39 | 0.9074 | 565.9 | 506.5 | |
| 1.45 | 3.34 | 1.70 | 3.94 | 9.70 | 126.01 | -65.73 | 82.15 | 0.9089 | 431.1 | 305.1 | |
| 17.26 | 56.65 | 21.34 | 70.21 | 10.19 | 124.72 | -67.02 | 81.56 | 0.9177 | 516.1 | 41.9 | |
| 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. | |