SDO HMI 2011-10-09 05:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.48 | 236.67 | 18.33 | 125.93 | 23.45 | 155.02 | 13.26 | 324.72 | 0.3666 | -953.4 | -422.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.02 | 0.00 | 1.11 | 24.58 | 160.80 | 19.04 | 317.10 | 0.4377 | -742.0 | -631.7 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 24.41 | 157.29 | 15.53 | 322.22 | 0.3997 | -693.0 | -529.3 | |
| 0.00 | 2.81 | 0.00 | 1.54 | 27.45 | 156.63 | 14.87 | 327.99 | 0.4314 | -773.0 | -569.0 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 27.62 | 156.55 | 14.78 | 328.35 | 0.4328 | -632.0 | -531.0 | |
| 6.23 | 222.02 | 3.31 | 118.00 | 23.11 | 155.32 | 13.56 | 323.56 | 0.3646 | -1254.0 | -436.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 21.52 | 154.96 | 13.20 | 321.32 | 0.3415 | -694.0 | -551.1 | |
| 28.25 | -5.00 | 15.02 | -5.00 | 23.33 | 155.01 | 13.25 | 324.57 | 0.3645 | -1474.1 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 25.31 | 152.75 | 10.98 | 332.27 | 0.3717 | -715.0 | -575.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 24.71 | 152.52 | 10.76 | 331.90 | 0.3617 | -703.0 | -541.5 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 22.68 | 151.86 | 10.10 | 330.31 | 0.3280 | 780.0 | 542.1 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 22.28 | 151.60 | 9.84 | 330.27 | 0.3203 | 811.0 | 516.7 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 25.95 | 147.99 | 6.22 | 343.87 | 0.3524 | 934.0 | 757.7 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 34.72 | 144.62 | 2.86 | 355.07 | 0.4799 | 754.0 | 591.9 | |
| 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. | |