| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.14 | 176.53 | 18.35 | 111.10 | 28.36 | 41.84 | 29.66 | 315.08 | 0.6189 | -834.3 | -360.7 | |
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back to the solar disc SDO HMI 2011-11-15 08:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.82 | 163.11 | 4.94 | 102.77 | 28.43 | 42.19 | 30.01 | 314.87 | 0.6228 | -967.4 | -357.4 | |
| 15.73 | -1.00 | 9.90 | -1.00 | 28.14 | 42.06 | 29.88 | 314.59 | 0.6192 | -1233.0 | 999999 | |
| 2.41 | -1.00 | 1.51 | -1.00 | 28.48 | 41.69 | 29.52 | 315.34 | 0.6184 | -962.0 | 999999 | |
| 3.18 | -1.00 | 2.00 | -1.00 | 28.71 | 41.61 | 29.43 | 315.71 | 0.6196 | -728.3 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.09 | 29.25 | 41.47 | 29.29 | 316.52 | 0.6227 | -630.0 | -513.2 | |
| 0.00 | 3.01 | 0.00 | 1.89 | 28.72 | 41.23 | 29.05 | 316.06 | 0.6160 | -790.0 | -717.8 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 29.51 | 41.39 | 29.22 | 316.92 | 0.6243 | -321.0 | -257.7 | |
| 0.00 | 0.95 | 0.00 | 0.59 | 29.01 | 40.19 | 28.02 | 317.35 | 0.6086 | -844.0 | -660.2 | |
| 0.00 | 1.98 | 0.00 | 1.23 | 29.89 | 39.30 | 27.12 | 319.30 | 0.6084 | -649.0 | -530.5 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 29.83 | 38.98 | 26.80 | 319.53 | 0.6049 | -712.0 | -660.7 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 29.67 | 38.85 | 26.68 | 319.45 | 0.6022 | -719.0 | -606.9 | |
| 0.00 | 0.69 | 0.00 | 0.43 | 30.27 | 38.87 | 26.70 | 320.17 | 0.6080 | -552.0 | -496.8 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 27.18 | 36.45 | 24.27 | 318.68 | 0.5560 | 796.0 | 659.3 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 27.37 | 36.38 | 24.21 | 319.01 | 0.5573 | 663.0 | 538.8 | |
| 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. | |