| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.80 | 29.68 | 0.95 | 15.77 | 17.78 | 214.90 | 12.99 | 323.31 | 0.3586 | 477.0 | 453.0 | |
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back to the solar disc SDO HMI 2011-11-28 06:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.60 | 17.83 | 219.02 | 17.11 | 315.59 | 0.4019 | 801.0 | 633.5 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.07 | 218.62 | 16.71 | 316.69 | 0.4002 | 972.0 | 714.2 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 16.35 | 218.08 | 16.16 | 314.34 | 0.3751 | -961.0 | -800.0 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 17.80 | 217.27 | 15.36 | 318.53 | 0.3824 | 896.0 | 744.3 | |
| 0.00 | 2.91 | 0.00 | 1.58 | 19.73 | 217.42 | 15.50 | 321.59 | 0.4067 | 870.0 | 720.6 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 20.39 | 216.28 | 14.36 | 324.68 | 0.4039 | 941.0 | 800.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 15.79 | 215.64 | 13.73 | 317.73 | 0.3410 | -874.0 | -694.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 16.46 | 215.53 | 13.62 | 319.31 | 0.3478 | -722.0 | -554.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.20 | 215.04 | 13.13 | 321.72 | 0.3518 | -734.0 | -587.5 | |
| 0.00 | 2.14 | 0.00 | 1.13 | 17.42 | 213.95 | 12.04 | 324.47 | 0.3439 | 737.0 | 573.8 | |
| 0.00 | 2.82 | 0.00 | 1.49 | 17.39 | 213.54 | 11.62 | 325.34 | 0.3396 | 786.0 | 601.4 | |
| 1.80 | 2.48 | 0.95 | 1.31 | 17.82 | 213.28 | 11.36 | 326.67 | 0.3430 | 780.7 | 720.2 | |
| 0.00 | 3.25 | 0.00 | 1.71 | 17.39 | 213.12 | 11.21 | 326.29 | 0.3358 | 886.0 | 777.2 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 17.92 | 213.00 | 11.09 | 327.47 | 0.3417 | 898.0 | 760.3 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 17.76 | 212.93 | 11.01 | 327.38 | 0.3390 | 1169.0 | 883.0 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 17.52 | 212.47 | 10.56 | 328.05 | 0.3316 | 806.0 | 640.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.46 | 212.18 | 10.27 | 328.65 | 0.3283 | 872.0 | 693.1 | |
| 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. | |