SDO HMI 2011-11-28 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.47 | 162.59 | 16.33 | 93.05 | 17.93 | 223.54 | 25.45 | 305.28 | 0.5031 | -455.9 | -370.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.74 | 15.32 | 225.64 | 27.55 | 298.83 | 0.5113 | 657.0 | 438.7 | |
| 9.92 | 41.29 | 5.71 | 23.76 | 17.79 | 224.32 | 26.23 | 304.28 | 0.5114 | -959.6 | -488.4 | |
| 18.55 | 102.76 | 10.62 | 58.82 | 18.04 | 223.53 | 25.44 | 305.46 | 0.5035 | -1129.8 | -439.4 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 15.77 | 223.03 | 24.94 | 301.91 | 0.4801 | 455.0 | 216.1 | |
| 0.00 | 3.68 | 0.00 | 2.08 | 16.29 | 222.93 | 24.84 | 302.96 | 0.4826 | -139.0 | -267.1 | |
| 0.00 | 2.14 | 0.00 | 1.20 | 16.23 | 222.72 | 24.63 | 303.06 | 0.4795 | 542.0 | 355.5 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 15.25 | 222.56 | 24.47 | 301.40 | 0.4702 | 947.0 | 810.7 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 15.71 | 222.41 | 24.33 | 302.40 | 0.4717 | 688.0 | 548.2 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 18.77 | 221.72 | 23.63 | 308.58 | 0.4875 | -351.0 | -462.2 | |
| 0.00 | 1.37 | 0.00 | 0.78 | 20.01 | 221.64 | 23.55 | 310.75 | 0.4976 | -837.0 | -652.2 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 19.67 | 221.38 | 23.29 | 310.48 | 0.4915 | -784.0 | -578.8 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 18.69 | 219.78 | 21.69 | 310.71 | 0.4638 | 736.0 | 664.1 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 20.91 | 219.55 | 21.47 | 314.67 | 0.4827 | 741.0 | 486.4 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 20.97 | 218.99 | 20.90 | 315.50 | 0.4772 | 796.0 | 548.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 21.40 | 217.09 | 19.00 | 318.75 | 0.4617 | 655.0 | 526.8 | |
| 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. | |