| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.72 | 38.25 | 5.99 | 19.56 | -20.37 | 67.79 | 3.27 | 192.35 | 0.2550 | -73.6 | 106.8 | |
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back to the solar disc SDO HMI 2011-02-11 19:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.59 | 10.01 | 1.84 | 5.13 | -20.19 | 71.59 | 7.07 | 206.18 | 0.2629 | 1015.1 | 855.9 | |
| 5.22 | 6.93 | 2.67 | 3.55 | -20.02 | 71.21 | 6.68 | 205.24 | 0.2574 | 1077.6 | 929.8 | |
| 0.00 | 2.91 | 0.00 | 1.49 | -20.48 | 70.88 | 6.35 | 203.39 | 0.2622 | 727.0 | 653.2 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -20.21 | 70.74 | 6.21 | 203.38 | 0.2571 | 1093.0 | 859.8 | |
| 0.00 | 1.20 | 0.00 | 0.61 | -20.18 | 69.91 | 5.39 | 200.61 | 0.2515 | 893.0 | 697.9 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -18.86 | 69.15 | 4.62 | 199.82 | 0.2260 | 702.0 | 462.5 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -20.82 | 64.52 | -0.01 | 179.98 | 0.2458 | -995.0 | -822.4 | |
| 2.91 | 3.76 | 1.48 | 1.92 | -19.94 | 64.20 | -0.32 | 178.69 | 0.2308 | -1127.3 | -955.2 | |
| 0.00 | 1.80 | 0.00 | 0.92 | -20.45 | 63.19 | -1.33 | 174.78 | 0.2406 | -841.0 | -896.8 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -21.19 | 62.84 | -1.69 | 173.76 | 0.2535 | -854.0 | -663.2 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -20.45 | 62.56 | -1.96 | 172.34 | 0.2418 | -899.0 | -523.1 | |
| 0.00 | 1.20 | 0.00 | 0.61 | -21.21 | 62.39 | -2.13 | 172.15 | 0.2549 | -843.0 | -646.7 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -21.61 | 62.39 | -2.14 | 172.35 | 0.2616 | -756.0 | -605.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -20.96 | 60.43 | -4.09 | 164.91 | 0.2573 | -983.0 | -797.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -21.39 | 60.42 | -4.11 | 165.32 | 0.2643 | -880.0 | -726.2 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -21.73 | 58.01 | -6.51 | 157.99 | 0.2825 | -839.0 | -572.5 | |
| 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. | |