SDO HMI 2014-09-09 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.56 | 66.17 | 20.35 | 44.25 | 9.70 | 147.27 | 42.59 | 276.46 | 0.6733 | 112.0 | -112.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.21 | 5.34 | 2.27 | 3.79 | 9.74 | 150.79 | 46.10 | 276.56 | 0.7172 | -671.3 | -462.9 | |
| 0.00 | 2.14 | 0.00 | 1.51 | 10.05 | 150.76 | 46.07 | 276.99 | 0.7168 | -623.0 | -552.2 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 10.64 | 150.03 | 45.34 | 277.81 | 0.7080 | -566.0 | -461.5 | |
| 0.80 | 26.01 | 0.55 | 17.64 | 10.16 | 148.52 | 43.83 | 277.14 | 0.6893 | -367.9 | -531.4 | |
| 5.17 | -4.00 | 3.51 | -4.00 | 10.06 | 148.24 | 43.56 | 277.00 | 0.6859 | -803.6 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.66 | 9.68 | 148.14 | 43.45 | 276.43 | 0.6845 | -708.0 | -548.5 | |
| 2.67 | -4.00 | 1.81 | -4.00 | 10.23 | 148.10 | 43.41 | 277.24 | 0.6841 | -713.4 | 999999 | |
| 1.51 | -4.00 | 1.02 | -4.00 | 10.25 | 147.89 | 43.21 | 277.27 | 0.6815 | -802.2 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.35 | 9.49 | 146.03 | 41.34 | 276.14 | 0.6575 | 182.0 | 157.0 | |
| 13.01 | 24.76 | 8.48 | 16.13 | 9.31 | 145.67 | 40.99 | 275.86 | 0.6529 | 720.9 | 504.1 | |
| 0.00 | 0.80 | 0.00 | 0.52 | 8.94 | 145.34 | 40.65 | 275.29 | 0.6486 | 547.0 | 428.3 | |
| 0.00 | 1.87 | 0.00 | 1.21 | 9.55 | 145.34 | 40.66 | 276.23 | 0.6486 | 796.0 | 725.0 | |
| 4.19 | -10.00 | 2.71 | -10.00 | 9.19 | 145.25 | 40.56 | 275.68 | 0.6474 | 925.2 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.86 | 8.97 | 144.98 | 40.29 | 275.33 | 0.6438 | 712.0 | 662.1 | |
| 0.00 | 1.87 | 0.00 | 1.21 | 9.16 | 144.93 | 40.24 | 275.62 | 0.6431 | 871.0 | 728.0 | |
| 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. | |