| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.32 | 63.70 | 10.01 | 34.72 | -16.47 | 266.95 | 16.69 | 221.51 | 0.4186 | 474.9 | 188.5 | |
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back to the solar disc SDO HMI 2011-11-24 14:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.58 | -15.63 | 272.42 | 22.16 | 230.78 | 0.4709 | 686.0 | 510.5 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -15.81 | 271.48 | 21.22 | 229.30 | 0.4613 | 814.0 | 636.4 | |
| 0.00 | 1.88 | 0.00 | 1.01 | -12.33 | 268.70 | 18.44 | 231.97 | 0.3940 | 662.0 | 606.6 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -12.42 | 268.13 | 17.87 | 230.94 | 0.3877 | 761.0 | 558.4 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -12.33 | 267.93 | 17.67 | 230.83 | 0.3843 | 988.0 | 859.4 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -12.75 | 267.64 | 17.39 | 229.50 | 0.3849 | 919.0 | 763.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -12.17 | 267.32 | 17.06 | 230.18 | 0.3750 | 688.0 | 668.2 | |
| 13.70 | 34.59 | 7.50 | 18.95 | -16.86 | 267.63 | 17.37 | 221.98 | 0.4291 | 1064.9 | 412.5 | |
| 0.00 | 1.88 | 0.00 | 1.02 | -15.54 | 266.10 | 15.84 | 221.64 | 0.3976 | 961.0 | 756.5 | |
| 2.31 | 3.77 | 1.25 | 2.04 | -16.50 | 265.79 | 15.54 | 219.47 | 0.4058 | -891.7 | -807.2 | |
| 1.80 | 2.40 | 0.98 | 1.31 | -18.84 | 264.94 | 14.68 | 214.37 | 0.4266 | 701.7 | 431.1 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -19.38 | 264.79 | 14.53 | 213.37 | 0.4322 | 768.0 | 644.9 | |
| 0.00 | 5.82 | 0.00 | 3.15 | -17.52 | 264.53 | 14.28 | 215.56 | 0.4061 | -919.0 | -825.0 | |
| 0.51 | 2.14 | 0.28 | 1.16 | -17.36 | 264.26 | 14.01 | 215.29 | 0.4016 | -1088.8 | -928.5 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -15.67 | 263.51 | 13.25 | 216.48 | 0.3728 | -711.0 | -571.2 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -15.67 | 263.16 | 12.90 | 215.77 | 0.3695 | -856.0 | -680.3 | |
| 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. | |