SDO HMI 2011-09-03 03:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.86 | 52.24 | 8.85 | 31.00 | 13.49 | 291.34 | 33.27 | 283.68 | 0.5514 | -208.4 | -314.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.49 | 14.12 | 293.66 | 35.59 | 284.21 | 0.5844 | -528.0 | -542.7 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 12.91 | 292.17 | 34.10 | 282.40 | 0.5616 | -533.0 | -433.7 | |
| 3.85 | 28.36 | 2.30 | 16.90 | 13.19 | 292.17 | 34.10 | 282.89 | 0.5622 | -789.8 | -629.5 | |
| 5.46 | 6.62 | 3.26 | 3.95 | 13.51 | 291.92 | 33.86 | 283.52 | 0.5593 | -870.4 | -732.3 | |
| 1.97 | 5.19 | 1.17 | 3.10 | 14.06 | 291.90 | 33.83 | 284.50 | 0.5600 | -610.8 | -710.2 | |
| 1.79 | -3.00 | 1.06 | -3.00 | 13.10 | 291.71 | 33.64 | 282.82 | 0.5555 | -985.8 | 999999 | |
| 1.79 | -3.00 | 1.06 | -3.00 | 13.23 | 291.54 | 33.47 | 283.10 | 0.5534 | -996.2 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.95 | 10.90 | 290.77 | 32.71 | 278.97 | 0.5392 | 764.0 | 618.8 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 10.13 | 290.57 | 32.50 | 277.54 | 0.5357 | 695.0 | 606.7 | |
| 0.00 | 1.43 | 0.00 | 0.84 | 9.90 | 290.40 | 32.33 | 277.12 | 0.5330 | 767.0 | 586.2 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 15.52 | 288.41 | 30.34 | 288.28 | 0.5146 | 481.0 | 452.2 | |
| 0.00 | 2.86 | 0.00 | 1.65 | 15.88 | 287.96 | 29.89 | 289.17 | 0.5095 | 719.0 | 543.8 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 17.30 | 287.40 | 29.33 | 292.15 | 0.5070 | 656.0 | 481.3 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 16.27 | 287.08 | 29.01 | 290.32 | 0.4985 | 728.0 | 585.8 | |
| 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. | |