| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.34 | 280.37 | 33.34 | 206.44 | 17.49 | 222.95 | -45.95 | 67.90 | 0.7422 | -574.3 | -216.1 | |
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back to the solar disc SDO HMI 2011-11-23 04:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.80 | 250.28 | 23.22 | 183.58 | 17.44 | 223.40 | -45.50 | 67.83 | 0.7372 | -1100.7 | -280.6 | |
| 9.86 | -1.00 | 7.34 | -1.00 | 17.95 | 222.47 | -46.43 | 67.46 | 0.7487 | -627.7 | 999999 | |
| 0.00 | 2.23 | 0.00 | 1.68 | 18.74 | 221.92 | -46.99 | 66.61 | 0.7568 | -421.0 | -273.5 | |
| 0.00 | 1.80 | 0.00 | 1.36 | 18.02 | 221.76 | -47.15 | 67.58 | 0.7565 | 58.0 | -54.2 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 19.77 | 220.77 | -48.13 | 65.65 | 0.7715 | 648.0 | 544.4 | |
| 0.51 | 10.97 | 0.39 | 8.25 | 16.54 | 221.75 | -47.15 | 69.50 | 0.7527 | -284.8 | 246.6 | |
| 0.00 | 5.40 | 0.00 | 4.02 | 15.96 | 221.94 | -46.97 | 70.20 | 0.7493 | 289.0 | 216.6 | |
| 3.17 | -6.00 | 2.39 | -6.00 | 16.47 | 221.50 | -47.40 | 69.65 | 0.7552 | 385.0 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.51 | 16.92 | 220.71 | -48.20 | 69.30 | 0.7648 | 653.0 | 555.0 | |
| 0.00 | 1.20 | 0.00 | 0.91 | 16.18 | 220.77 | -48.14 | 70.23 | 0.7624 | 789.0 | 631.8 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 16.38 | 220.33 | -48.58 | 70.08 | 0.7675 | 666.0 | 585.2 | |
| 0.00 | 2.14 | 0.00 | 1.70 | 17.56 | 219.10 | -49.80 | 68.90 | 0.7829 | 645.0 | 547.7 | |
| 0.00 | 1.63 | 0.00 | 1.29 | 17.22 | 219.13 | -49.78 | 69.32 | 0.7818 | 543.0 | 430.8 | |
| 0.00 | 1.03 | 0.00 | 0.82 | 17.82 | 218.61 | -50.30 | 68.69 | 0.7884 | 309.0 | 243.1 | |
| 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. | |