SDO HMI 2011-08-30 01:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.72 | 283.52 | 23.72 | 150.79 | 13.98 | 291.50 | -20.50 | 69.67 | 0.3642 | -608.0 | -318.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.88 | 0.00 | 1.00 | 18.44 | 292.74 | -19.26 | 57.14 | 0.3742 | 744.0 | 589.7 | |
| 39.16 | 266.31 | 20.77 | 141.29 | 13.79 | 291.81 | -20.19 | 69.86 | 0.3585 | -1325.4 | -392.6 | |
| 5.56 | -2.00 | 2.95 | -2.00 | 13.63 | 291.49 | -20.51 | 70.54 | 0.3626 | -1015.2 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 14.71 | 289.13 | -22.87 | 69.45 | 0.4031 | 946.0 | 703.6 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 12.04 | 288.86 | -23.14 | 76.13 | 0.3975 | 740.0 | 682.7 | |
| 0.00 | 2.96 | 0.00 | 1.60 | 14.08 | 288.62 | -23.38 | 71.29 | 0.4080 | 834.0 | 706.2 | |
| 0.00 | 2.78 | 0.00 | 1.52 | 14.34 | 287.78 | -24.23 | 71.17 | 0.4218 | 741.0 | 610.1 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 20.43 | 286.54 | -25.46 | 59.14 | 0.4713 | 717.0 | 539.3 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 21.91 | 286.15 | -25.85 | 56.66 | 0.4861 | 706.0 | 579.3 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 21.78 | 286.00 | -26.00 | 57.04 | 0.4872 | 713.0 | 575.3 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 15.79 | 286.70 | -25.30 | 68.56 | 0.4437 | 788.0 | 659.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 21.54 | 285.72 | -26.28 | 57.70 | 0.4892 | 795.0 | 627.2 | |
| 0.00 | 1.52 | 0.00 | 0.85 | 14.89 | 285.45 | -26.55 | 71.18 | 0.4582 | 360.0 | 356.5 | |
| 0.00 | 1.43 | 0.00 | 0.85 | 23.56 | 282.26 | -29.74 | 56.82 | 0.5455 | 720.0 | 541.4 | |
| 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. | |