| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.74 | 195.01 | 16.44 | 116.25 | 19.56 | 104.24 | -28.51 | 54.15 | 0.5575 | -710.3 | -333.9 | |
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back to the solar disc SDO HMI 2011-12-03 12:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.60 | 19.78 | 106.93 | -25.81 | 51.20 | 0.5278 | 596.0 | 463.5 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 24.94 | 104.51 | -28.23 | 46.08 | 0.5977 | -766.0 | -590.2 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 17.38 | 105.00 | -27.74 | 56.90 | 0.5325 | 733.0 | 626.3 | |
| 27.74 | 177.36 | 16.44 | 105.11 | 19.05 | 104.46 | -28.29 | 54.67 | 0.5512 | -1096.3 | -348.9 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 27.85 | 101.83 | -30.92 | 44.70 | 0.6481 | -472.0 | -392.5 | |
| 0.00 | 1.62 | 0.00 | 1.03 | 25.48 | 102.31 | -30.44 | 47.31 | 0.6245 | -654.0 | -541.5 | |
| 0.00 | 1.79 | 0.00 | 1.14 | 26.13 | 102.12 | -30.62 | 46.62 | 0.6315 | -592.0 | -516.8 | |
| 0.00 | 1.79 | 0.00 | 1.14 | 25.87 | 102.12 | -30.62 | 46.96 | 0.6294 | -784.0 | -603.3 | |
| 0.00 | 1.02 | 0.00 | 0.65 | 26.20 | 101.91 | -30.83 | 46.71 | 0.6341 | -609.0 | -527.6 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 24.96 | 102.15 | -30.59 | 48.13 | 0.6219 | -675.0 | -536.6 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 30.17 | 99.87 | -32.87 | 43.49 | 0.6842 | -668.0 | -550.5 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 17.96 | 102.84 | -29.90 | 57.73 | 0.5631 | 871.0 | 741.0 | |
| 0.00 | 2.05 | 0.00 | 1.40 | 30.03 | 99.06 | -33.68 | 44.26 | 0.6903 | -549.0 | -502.5 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 15.09 | 100.58 | -32.16 | 63.92 | 0.5744 | 680.0 | 553.6 | |
| 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. | |