SDO HMI 2011-10-23 22:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.09 | 0.00 | 7.99 | 24.09 | 330.36 | 22.62 | 313.38 | 0.4869 | -538.7 | -480.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.65 | 0.00 | 0.97 | 22.35 | 336.06 | 28.32 | 304.79 | 0.5364 | -834.0 | -668.1 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 21.36 | 332.38 | 24.64 | 306.39 | 0.4843 | -807.0 | -661.4 | |
| 0.00 | 0.26 | 0.00 | 0.15 | 22.43 | 331.44 | 23.70 | 309.22 | 0.4816 | -461.0 | -352.0 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 22.75 | 331.29 | 23.55 | 309.94 | 0.4825 | -779.0 | -642.6 | |
| 0.00 | 1.39 | 0.00 | 0.78 | 22.50 | 331.21 | 23.47 | 309.60 | 0.4794 | -982.0 | -807.9 | |
| 0.00 | 1.65 | 0.00 | 0.93 | 23.93 | 329.88 | 22.14 | 313.53 | 0.4771 | -774.0 | -618.3 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 23.77 | 329.75 | 22.01 | 313.43 | 0.4742 | -851.0 | -716.7 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 24.69 | 329.92 | 22.18 | 314.73 | 0.4847 | -814.0 | -588.6 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 25.01 | 329.87 | 22.13 | 315.30 | 0.4873 | -643.0 | -547.3 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 24.12 | 329.67 | 21.93 | 314.10 | 0.4766 | -748.0 | -620.8 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 24.80 | 329.48 | 21.74 | 315.43 | 0.4810 | -703.0 | -605.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 28.59 | 324.87 | 17.13 | 327.15 | 0.4788 | 621.0 | 540.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 28.44 | 324.63 | 16.89 | 327.30 | 0.4749 | 772.0 | 620.5 | |
| 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. | |