SDO HMI 2011-02-26 11:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.22 | 154.09 | 31.14 | 282.22 | 26.53 | 163.33 | -68.07 | 59.71 | 0.9623 | -118.0 | -207.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.96 | 0.00 | 5.41 | 24.77 | 168.78 | -62.62 | 59.88 | 0.9337 | -454.0 | -362.6 | |
| 0.00 | 1.21 | 0.00 | 1.92 | 26.56 | 165.76 | -65.63 | 58.99 | 0.9520 | -416.0 | -320.1 | |
| 3.53 | 137.46 | 6.65 | 254.03 | 27.82 | 162.83 | -68.57 | 58.56 | 0.9661 | -434.5 | -235.0 | |
| 0.00 | 1.03 | 0.00 | 1.50 | 24.13 | 167.00 | -64.39 | 61.07 | 0.9418 | -159.0 | -129.2 | |
| 0.00 | 1.81 | 0.00 | 3.01 | 25.97 | 164.69 | -66.71 | 59.89 | 0.9559 | 275.0 | 276.3 | |
| 0.00 | 0.95 | 0.00 | 1.84 | 27.75 | 162.26 | -69.13 | 58.78 | 0.9682 | 25.0 | 25.1 | |
| 4.82 | -3.00 | 8.97 | -3.00 | 26.82 | 162.77 | -68.63 | 59.56 | 0.9651 | -594.7 | 999999 | |
| 7.23 | -3.00 | 12.59 | -3.00 | 26.01 | 163.78 | -67.62 | 60.10 | 0.9598 | 336.2 | 999999 | |
| 0.00 | 1.81 | 0.00 | 3.56 | 27.42 | 161.87 | -69.53 | 59.21 | 0.9692 | 78.0 | 17.7 | |
| 1.64 | -3.00 | 2.93 | -3.00 | 26.21 | 163.27 | -68.12 | 60.04 | 0.9622 | -220.9 | 999999 | |
| 0.00 | 2.76 | 0.00 | 5.16 | 24.92 | 162.12 | -69.28 | 61.63 | 0.9652 | 434.0 | 330.0 | |
| 0.00 | 1.29 | 0.00 | 2.52 | 24.89 | 161.30 | -70.09 | 61.87 | 0.9683 | 101.0 | 103.6 | |
| 0.00 | 1.81 | 0.00 | 3.27 | 23.65 | 162.35 | -69.05 | 62.84 | 0.9627 | 19.0 | 21.7 | |
| 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. | |