| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.17 | 287.54 | 42.53 | 259.05 | 9.47 | 55.54 | -56.62 | 81.09 | 0.8348 | -625.6 | -243.4 | |
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back to the solar disc SDO HMI 2011-11-07 18:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.57 | 238.15 | 25.60 | 208.06 | 9.25 | 56.93 | -55.23 | 81.31 | 0.8223 | -959.9 | -221.2 | |
| 3.79 | 6.29 | 3.37 | 5.60 | 12.01 | 56.00 | -56.15 | 78.03 | 0.8326 | 431.1 | 126.8 | |
| 0.00 | 1.38 | 0.00 | 1.21 | 10.34 | 56.44 | -55.71 | 80.01 | 0.8275 | -306.0 | -282.4 | |
| 0.00 | 0.60 | 0.00 | 0.53 | 10.90 | 56.23 | -55.92 | 79.35 | 0.8298 | -367.0 | -328.7 | |
| 1.29 | -1.00 | 1.13 | -1.00 | 8.82 | 56.66 | -55.50 | 81.85 | 0.8249 | -527.8 | 999999 | |
| 4.22 | -1.00 | 3.72 | -1.00 | 9.40 | 56.25 | -55.90 | 81.16 | 0.8290 | -379.8 | 999999 | |
| 4.91 | -1.00 | 4.34 | -1.00 | 9.70 | 56.18 | -55.98 | 80.81 | 0.8298 | -418.7 | 999999 | |
| 1.29 | -1.00 | 1.14 | -1.00 | 8.77 | 56.29 | -55.86 | 81.92 | 0.8284 | -273.3 | 999999 | |
| 0.00 | 2.33 | 0.00 | 2.12 | 11.17 | 55.05 | -57.11 | 79.10 | 0.8411 | -626.0 | -434.8 | |
| 3.10 | 31.56 | 3.23 | 32.70 | 9.38 | 50.39 | -61.77 | 81.35 | 0.8812 | -721.9 | -502.4 | |
| 0.00 | 2.41 | 0.00 | 2.55 | 9.80 | 49.93 | -62.23 | 80.87 | 0.8850 | -260.0 | -177.1 | |
| 0.00 | 0.60 | 0.00 | 0.77 | 12.61 | 44.62 | -67.54 | 77.88 | 0.9240 | 359.0 | 377.3 | |
| 0.00 | 4.22 | 0.00 | 5.51 | 12.77 | 44.21 | -67.95 | 77.72 | 0.9267 | 428.0 | 271.2 | |
| 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. | |