SDO HMI 2011-11-13 10:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.16 | 375.11 | 28.51 | 212.77 | 16.21 | 63.86 | 26.41 | 298.69 | 0.4890 | -751.4 | -358.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.16 | 352.85 | 28.51 | 200.52 | 16.05 | 64.23 | 26.78 | 297.99 | 0.4924 | -1336.3 | -407.0 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 18.74 | 64.66 | 27.21 | 302.49 | 0.5154 | -656.0 | -540.5 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 14.12 | 62.40 | 24.95 | 295.65 | 0.4558 | -805.0 | -663.4 | |
| 0.00 | 1.81 | 0.00 | 1.01 | 17.07 | 62.17 | 24.72 | 301.68 | 0.4718 | -889.0 | -646.4 | |
| 0.00 | 2.75 | 0.00 | 1.52 | 17.98 | 59.65 | 22.20 | 306.01 | 0.4462 | 660.0 | 603.1 | |
| 0.00 | 1.89 | 0.00 | 1.05 | 18.69 | 59.71 | 22.26 | 307.27 | 0.4529 | 811.0 | 646.2 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 17.93 | 57.80 | 20.35 | 308.12 | 0.4224 | 865.0 | 666.9 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 16.44 | 56.88 | 19.43 | 306.29 | 0.3975 | 798.0 | 607.5 | |
| 0.00 | 1.46 | 0.00 | 0.80 | 18.41 | 56.76 | 19.31 | 310.43 | 0.4141 | 682.0 | 599.4 | |
| 0.00 | 2.32 | 0.00 | 1.27 | 21.06 | 55.79 | 18.34 | 316.68 | 0.4298 | 700.0 | 576.1 | |
| 0.00 | 1.29 | 0.00 | 0.71 | 22.73 | 54.97 | 17.52 | 320.67 | 0.4399 | 800.0 | 591.1 | |
| 0.00 | 1.46 | 0.00 | 0.80 | 21.49 | 54.41 | 16.96 | 319.53 | 0.4199 | 939.0 | 755.2 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 21.31 | 53.69 | 16.24 | 320.41 | 0.4105 | 749.0 | 487.1 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 18.17 | 52.13 | 14.68 | 317.43 | 0.3575 | 733.0 | 546.9 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 19.86 | 49.85 | 12.40 | 325.15 | 0.3551 | 771.0 | 588.5 | |
| 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. | |