SDO HMI 2011-02-11 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.58 | 40.50 | 6.41 | 20.68 | -20.17 | 67.93 | -1.55 | 174.39 | 0.2434 | 117.7 | -149.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 12.50 | 0.83 | 6.36 | -20.13 | 71.21 | 1.73 | 186.91 | 0.2361 | 974.1 | 798.3 | |
| 5.73 | -1.00 | 2.92 | -1.00 | -19.95 | 71.17 | 1.69 | 186.88 | 0.2330 | 1119.5 | 999999 | |
| 5.22 | 8.47 | 2.66 | 4.32 | -20.19 | 70.70 | 1.22 | 184.88 | 0.2363 | 1074.2 | 810.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -20.93 | 70.14 | 0.66 | 182.49 | 0.2481 | 800.0 | 600.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -20.29 | 69.95 | 0.47 | 181.85 | 0.2371 | 964.0 | 866.8 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -18.77 | 67.98 | -1.51 | 173.24 | 0.2126 | 910.0 | 722.6 | |
| 0.00 | 1.80 | 0.00 | 0.92 | -20.18 | 65.22 | -4.26 | 163.42 | 0.2457 | -852.0 | -633.3 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -20.87 | 64.59 | -4.89 | 162.09 | 0.2600 | -863.0 | -693.2 | |
| 0.00 | 5.82 | 0.00 | 2.98 | -20.05 | 64.24 | -5.24 | 159.73 | 0.2488 | -1299.0 | -976.3 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -20.53 | 64.10 | -5.38 | 159.94 | 0.2573 | -932.0 | -762.4 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -20.56 | 63.49 | -5.99 | 157.95 | 0.2613 | -876.0 | -654.1 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -20.61 | 63.21 | -6.28 | 157.09 | 0.2641 | -964.0 | -774.0 | |
| 0.00 | 2.74 | 0.00 | 1.41 | -20.42 | 62.61 | -6.87 | 154.87 | 0.2652 | -889.0 | -727.5 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -20.41 | 61.37 | -8.11 | 151.04 | 0.2744 | -884.0 | -650.0 | |
| 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. | |