| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.02 | 330.34 | 26.05 | 183.57 | 28.15 | 43.79 | -10.66 | 21.08 | 0.4546 | -986.7 | -426.3 | |
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back to the solar disc SDO HMI 2011-11-12 03:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.19 | 0.00 | 1.80 | 31.27 | 46.49 | -7.96 | 14.12 | 0.4873 | -872.0 | -738.7 | |
| 0.00 | 1.29 | 0.00 | 0.76 | 33.70 | 43.74 | -10.72 | 16.94 | 0.5331 | -667.0 | -525.1 | |
| 44.01 | 315.27 | 24.38 | 174.73 | 27.93 | 44.03 | -10.42 | 20.89 | 0.4501 | -1335.0 | -440.3 | |
| 1.29 | -3.00 | 0.72 | -3.00 | 28.39 | 43.95 | -10.50 | 20.63 | 0.4571 | -775.1 | 999999 | |
| 1.12 | -3.00 | 0.62 | -3.00 | 28.02 | 43.34 | -11.12 | 22.05 | 0.4554 | -807.4 | 999999 | |
| 0.60 | -3.00 | 0.33 | -3.00 | 27.96 | 43.21 | -11.25 | 22.34 | 0.4552 | -701.6 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.31 | 36.66 | 41.37 | -13.09 | 18.21 | 0.5834 | -671.0 | -507.7 | |
| 0.00 | 1.72 | 0.00 | 1.06 | 37.04 | 40.54 | -13.92 | 19.00 | 0.5922 | -606.0 | -501.0 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 28.26 | 41.25 | -13.21 | 25.37 | 0.4717 | -958.0 | -787.1 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 24.50 | 37.97 | -16.49 | 35.29 | 0.4489 | 814.0 | 608.7 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 27.42 | 37.09 | -17.37 | 32.75 | 0.4920 | 646.0 | 499.1 | |
| 0.00 | 2.07 | 0.00 | 1.22 | 30.21 | 34.31 | -20.15 | 33.10 | 0.5473 | 633.0 | 427.9 | |
| 0.00 | 1.64 | 0.00 | 1.00 | 32.99 | 32.68 | -21.78 | 31.91 | 0.5910 | 648.0 | 537.2 | |
| 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. | |