| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.21 | 65.85 | 9.29 | 35.37 | -16.19 | 266.93 | 13.93 | 217.07 | 0.3875 | 478.6 | 213.1 | |
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back to the solar disc SDO HMI 2011-11-24 09:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.23 | 0.00 | 1.18 | -11.82 | 269.47 | 16.47 | 229.93 | 0.3643 | 748.0 | 539.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -12.09 | 268.57 | 15.58 | 227.79 | 0.3561 | 783.0 | 569.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -15.97 | 268.75 | 15.75 | 220.72 | 0.4019 | 789.0 | 575.7 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -12.48 | 268.09 | 15.10 | 226.08 | 0.3546 | 697.0 | 591.4 | |
| 0.00 | 1.88 | 0.00 | 1.00 | -12.39 | 267.90 | 14.90 | 225.91 | 0.3513 | 976.0 | 725.0 | |
| 0.00 | 4.45 | 0.00 | 2.36 | -12.90 | 267.59 | 14.59 | 224.24 | 0.3535 | 828.0 | 755.6 | |
| 14.30 | 36.40 | 7.73 | 19.67 | -16.89 | 267.58 | 14.58 | 217.08 | 0.4013 | 1105.3 | 436.3 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -14.96 | 267.15 | 14.15 | 219.49 | 0.3731 | 693.0 | 465.0 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -15.45 | 266.05 | 13.05 | 216.42 | 0.3682 | 782.0 | 711.4 | |
| 1.28 | 4.28 | 0.69 | 2.29 | -16.50 | 265.74 | 12.74 | 214.08 | 0.3790 | -939.6 | -846.5 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -19.17 | 264.91 | 11.91 | 208.67 | 0.4080 | 698.0 | 575.3 | |
| 0.00 | 4.63 | 0.00 | 2.47 | -17.43 | 264.37 | 11.38 | 209.85 | 0.3799 | -720.0 | -803.1 | |
| 1.63 | 2.06 | 0.87 | 1.10 | -17.24 | 264.08 | 11.08 | 209.46 | 0.3748 | -1036.4 | -898.6 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -17.77 | 263.86 | 10.86 | 208.27 | 0.3806 | -935.0 | -779.7 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -15.68 | 263.08 | 10.08 | 209.41 | 0.3449 | -966.0 | -782.3 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -19.47 | 261.99 | 9.00 | 202.18 | 0.3922 | -698.0 | -519.8 | |
| 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. | |