SDO HMI 2011-10-22 04:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.64 | 0.00 | 10.92 | 25.32 | 329.88 | -0.94 | 1.66 | 0.3488 | -407.8 | -317.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.41 | 23.23 | 336.77 | 5.94 | 342.81 | 0.3235 | -802.0 | -614.6 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 23.17 | 336.37 | 5.55 | 343.83 | 0.3207 | -848.0 | -657.6 | |
| 0.00 | 1.48 | 0.00 | 0.77 | 22.43 | 334.82 | 4.00 | 347.64 | 0.3025 | -718.0 | -530.8 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 25.37 | 333.19 | 2.37 | 353.78 | 0.3461 | -805.0 | -661.6 | |
| 0.00 | 1.57 | 0.00 | 0.82 | 23.85 | 332.51 | 1.69 | 355.15 | 0.3201 | -905.0 | -712.7 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 25.24 | 331.87 | 1.05 | 357.22 | 0.3424 | -718.0 | -550.1 | |
| 0.00 | 3.05 | 0.00 | 1.60 | 24.89 | 329.60 | -1.23 | 3.32 | 0.3368 | -860.0 | -702.8 | |
| 0.00 | 3.66 | 0.00 | 1.93 | 25.24 | 329.50 | -1.33 | 3.52 | 0.3426 | -762.0 | -611.8 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 24.89 | 329.40 | -1.42 | 3.85 | 0.3370 | -602.0 | -487.7 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 27.13 | 329.27 | -1.55 | 3.71 | 0.3736 | -713.0 | -586.1 | |
| 0.00 | 1.83 | 0.00 | 0.99 | 27.85 | 325.20 | -5.62 | 12.73 | 0.3946 | 1006.0 | 798.4 | |
| 0.00 | 1.83 | 0.00 | 0.99 | 28.23 | 324.84 | -5.98 | 13.26 | 0.4019 | 679.0 | 546.2 | |
| 0.00 | 1.22 | 0.00 | 0.65 | 26.34 | 322.76 | -8.06 | 19.27 | 0.3823 | 747.0 | 606.2 | |
| 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. | |