SDO HMI 2014-07-08 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.86 | 0.00 | 13.33 | -22.65 | 200.48 | -17.69 | 147.78 | 0.5258 | 157.5 | 177.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.86 | -20.97 | 206.28 | -11.89 | 155.15 | 0.4598 | 836.0 | 734.7 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -21.76 | 205.03 | -13.14 | 153.73 | 0.4789 | 674.0 | 515.5 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -20.85 | 204.81 | -13.36 | 152.43 | 0.4682 | 766.0 | 648.5 | |
| 0.00 | 2.36 | 0.00 | 1.34 | -21.72 | 203.28 | -14.89 | 150.77 | 0.4909 | 940.0 | 617.4 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -21.96 | 203.15 | -15.02 | 150.82 | 0.4949 | 936.0 | 666.2 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.82 | 202.87 | -15.30 | 147.93 | 0.4696 | 725.0 | 565.1 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -27.09 | 200.24 | -17.93 | 151.69 | 0.5800 | -699.0 | -566.7 | |
| 0.00 | 1.63 | 0.00 | 0.99 | -26.95 | 200.12 | -18.05 | 151.40 | 0.5791 | -785.0 | -645.4 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -26.47 | 199.70 | -18.47 | 150.39 | 0.5762 | -756.0 | -580.3 | |
| 0.00 | 3.63 | 0.00 | 2.13 | -22.70 | 199.30 | -18.87 | 145.92 | 0.5345 | 830.0 | 736.2 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -22.84 | 199.17 | -19.00 | 145.90 | 0.5372 | 701.0 | 604.0 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -21.60 | 195.67 | -22.50 | 139.89 | 0.5544 | -539.0 | -411.7 | |
| 0.00 | 2.45 | 0.00 | 1.45 | -20.94 | 195.21 | -22.96 | 138.49 | 0.5519 | -652.0 | -490.9 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -21.05 | 193.55 | -24.62 | 136.71 | 0.5692 | -772.0 | -637.4 | |
| 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. | |