| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.93 | 178.15 | 17.27 | 110.89 | 19.55 | 104.38 | -32.73 | 57.47 | 0.6071 | -770.2 | -371.0 | |
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back to the solar disc SDO HMI 2011-12-03 04:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.97 | 25.06 | 106.13 | -30.98 | 48.35 | 0.6263 | -661.0 | -488.8 | |
| 0.00 | 0.68 | 0.00 | 0.41 | 20.09 | 107.02 | -30.09 | 54.64 | 0.5796 | 532.0 | 529.6 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 24.83 | 104.47 | -32.64 | 49.97 | 0.6416 | -819.0 | -603.3 | |
| 0.00 | 1.79 | 0.00 | 1.15 | 23.53 | 104.00 | -33.11 | 52.06 | 0.6374 | -735.0 | -550.6 | |
| 0.00 | 1.71 | 0.00 | 1.09 | 23.05 | 103.90 | -33.21 | 52.79 | 0.6351 | -607.0 | -566.5 | |
| 27.93 | 160.30 | 17.27 | 99.17 | 18.98 | 104.58 | -32.53 | 58.13 | 0.6011 | -1139.6 | -382.5 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 22.38 | 103.66 | -33.45 | 53.88 | 0.6332 | 789.0 | 689.6 | |
| 0.00 | 1.20 | 0.00 | 0.80 | 25.92 | 102.39 | -34.72 | 50.07 | 0.6704 | -814.0 | -678.5 | |
| 0.00 | 1.71 | 0.00 | 1.15 | 26.65 | 102.06 | -35.05 | 49.39 | 0.6785 | -597.0 | -448.9 | |
| 0.00 | 1.71 | 0.00 | 1.15 | 26.18 | 101.98 | -35.13 | 50.03 | 0.6762 | -529.0 | -425.8 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 24.49 | 102.18 | -34.93 | 52.07 | 0.6629 | -571.0 | -507.9 | |
| 0.00 | 1.79 | 0.00 | 1.30 | 30.08 | 98.91 | -38.20 | 47.33 | 0.7303 | -693.0 | -496.3 | |
| 0.00 | 1.02 | 0.00 | 0.66 | 18.40 | 100.46 | -36.65 | 61.55 | 0.6466 | 579.0 | 492.2 | |
| 0.00 | 1.11 | 0.00 | 0.73 | 18.11 | 99.40 | -37.72 | 62.53 | 0.6576 | 493.0 | 431.7 | |
| 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. | |