| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.94 | 51.46 | 11.10 | 40.92 | 8.55 | 347.62 | -51.47 | 81.52 | 0.7840 | 217.7 | 197.2 | |
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back to the solar disc SDO HMI 2011-11-13 07:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.34 | 4.13 | 0.26 | 3.15 | 7.92 | 349.64 | -49.45 | 82.21 | 0.7619 | -637.5 | -493.4 | |
| 0.00 | 1.98 | 0.00 | 1.50 | 7.44 | 349.71 | -49.37 | 82.84 | 0.7608 | -149.0 | -218.7 | |
| 1.64 | 3.79 | 1.25 | 2.89 | 8.36 | 349.52 | -49.57 | 81.64 | 0.7635 | -554.7 | -361.6 | |
| 0.00 | 1.29 | 0.00 | 1.01 | 9.13 | 348.48 | -50.61 | 80.72 | 0.7754 | -391.0 | -290.9 | |
| 0.00 | 1.55 | 0.00 | 1.22 | 9.12 | 348.25 | -50.84 | 80.75 | 0.7780 | -440.0 | -319.2 | |
| 7.57 | 19.19 | 5.93 | 15.01 | 8.31 | 348.35 | -50.74 | 81.78 | 0.7764 | 743.7 | 577.8 | |
| 0.00 | 1.46 | 0.00 | 1.16 | 8.74 | 347.84 | -51.25 | 81.26 | 0.7822 | 481.0 | 373.8 | |
| 0.00 | 0.86 | 0.00 | 0.68 | 7.77 | 347.58 | -51.51 | 82.52 | 0.7845 | -332.0 | -298.5 | |
| 0.00 | 1.55 | 0.00 | 1.24 | 8.84 | 347.29 | -51.80 | 81.18 | 0.7881 | 564.0 | 461.6 | |
| 2.93 | 6.71 | 2.36 | 5.41 | 9.33 | 346.94 | -52.15 | 80.57 | 0.7921 | 583.6 | 620.2 | |
| 0.00 | 0.77 | 0.00 | 0.63 | 8.98 | 346.47 | -52.62 | 81.05 | 0.7968 | 485.0 | 465.8 | |
| 0.00 | 1.12 | 0.00 | 0.92 | 8.91 | 346.28 | -52.81 | 81.14 | 0.7987 | 566.0 | 474.0 | |
| 0.00 | 0.95 | 0.00 | 0.77 | 7.40 | 346.57 | -52.52 | 83.03 | 0.7951 | -310.0 | -314.2 | |
| 0.00 | 1.12 | 0.00 | 0.92 | 7.45 | 346.26 | -52.83 | 82.99 | 0.7983 | -478.0 | -345.0 | |
| 0.00 | 0.95 | 0.00 | 0.81 | 9.44 | 344.58 | -54.51 | 80.60 | 0.8163 | -274.0 | -222.4 | |
| 1.46 | 2.84 | 1.30 | 2.52 | 9.34 | 342.90 | -56.19 | 80.82 | 0.8326 | 665.2 | 511.8 | |
| 0.00 | 1.20 | 0.00 | 1.08 | 9.45 | 342.71 | -56.38 | 80.70 | 0.8345 | 370.0 | 327.4 | |
| 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. | |