| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.77 | 68.61 | 19.78 | 37.84 | 17.77 | 214.08 | -20.79 | 50.29 | 0.4410 | 324.4 | 102.4 | |
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back to the solar disc SDO HMI 2011-11-25 18:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.91 | 0.00 | 1.58 | 18.58 | 217.32 | -17.55 | 44.27 | 0.4111 | 867.0 | 721.9 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 18.98 | 217.25 | -17.62 | 43.68 | 0.4163 | 616.0 | 547.3 | |
| 7.62 | 11.72 | 4.14 | 6.37 | 17.18 | 215.90 | -18.97 | 49.01 | 0.4132 | -1050.9 | -811.9 | |
| 0.00 | 2.74 | 0.00 | 1.51 | 19.28 | 215.49 | -19.37 | 45.76 | 0.4390 | 668.0 | 676.6 | |
| 0.00 | 2.05 | 0.00 | 1.12 | 17.23 | 215.27 | -19.60 | 49.78 | 0.4214 | -648.0 | -639.8 | |
| 0.00 | 0.51 | 0.00 | 0.28 | 17.88 | 215.06 | -19.80 | 48.85 | 0.4300 | -752.0 | -622.0 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 17.29 | 215.10 | -19.77 | 49.90 | 0.4240 | -320.0 | -350.7 | |
| 0.00 | 2.65 | 0.00 | 1.45 | 17.91 | 214.96 | -19.91 | 48.94 | 0.4315 | -853.0 | -717.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 18.22 | 214.89 | -19.98 | 48.47 | 0.4354 | -619.0 | -499.1 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 15.76 | 215.16 | -19.70 | 52.82 | 0.4090 | -904.0 | -744.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 18.12 | 214.74 | -20.13 | 48.85 | 0.4363 | -617.0 | -506.5 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 18.02 | 213.55 | -21.32 | 50.56 | 0.4495 | 643.0 | 504.7 | |
| 0.94 | 1.28 | 0.52 | 0.71 | 18.02 | 213.25 | -21.62 | 50.94 | 0.4531 | 812.3 | 863.5 | |
| 27.21 | 37.65 | 15.12 | 20.92 | 17.80 | 212.88 | -21.99 | 51.78 | 0.4557 | 1047.2 | 695.0 | |
| 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. | |