SDO HMI 2014-09-08 22:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.14 | 41.08 | 8.86 | 23.76 | 9.37 | 147.43 | 31.20 | 276.12 | 0.5158 | 6.8 | 66.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.10 | 6.60 | 2.44 | 3.92 | 9.29 | 150.08 | 33.85 | 275.88 | 0.5547 | -792.7 | -626.4 | |
| 4.72 | 7.75 | 2.80 | 4.60 | 9.58 | 149.82 | 33.59 | 276.41 | 0.5510 | -871.0 | -660.1 | |
| 0.80 | 3.03 | 0.47 | 1.76 | 9.14 | 147.84 | 31.61 | 275.67 | 0.5221 | -822.7 | -627.4 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 10.08 | 147.87 | 31.64 | 277.47 | 0.5229 | -524.0 | -366.4 | |
| 0.00 | 1.87 | 0.00 | 1.08 | 10.16 | 147.49 | 31.25 | 277.67 | 0.5173 | 672.0 | 563.1 | |
| 2.67 | 4.81 | 1.53 | 2.76 | 8.82 | 146.67 | 30.44 | 275.08 | 0.5046 | -847.7 | -682.7 | |
| 0.00 | 2.32 | 0.00 | 1.32 | 8.98 | 145.70 | 29.46 | 275.42 | 0.4900 | 625.0 | 426.7 | |
| 2.85 | 4.81 | 1.62 | 2.73 | 9.65 | 145.58 | 29.35 | 276.81 | 0.4886 | 872.1 | 636.8 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 9.95 | 145.61 | 29.38 | 277.43 | 0.4892 | 654.0 | 477.5 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 8.97 | 145.27 | 29.04 | 275.43 | 0.4836 | 514.0 | 439.2 | |
| 0.00 | 1.78 | 0.00 | 1.01 | 9.76 | 145.21 | 28.97 | 277.08 | 0.4830 | 973.0 | 812.7 | |
| 0.00 | 0.62 | 0.00 | 0.35 | 9.89 | 145.18 | 28.95 | 277.34 | 0.4827 | 514.0 | 599.7 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 9.08 | 145.04 | 28.80 | 275.66 | 0.4800 | 532.0 | 573.5 | |
| 0.00 | 3.12 | 0.00 | 1.76 | 9.30 | 144.85 | 28.61 | 276.14 | 0.4773 | 868.0 | 621.6 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 7.85 | 142.70 | 26.46 | 273.05 | 0.4439 | 774.0 | 625.8 | |
| 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. | |