| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.70 | 124.05 | 23.14 | 99.97 | 15.75 | 233.31 | 50.61 | 289.24 | 0.7900 | -701.9 | -230.5 | |
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back to the solar disc SDO HMI 2011-11-29 17:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.95 | 17.67 | 235.48 | 52.78 | 291.07 | 0.8153 | -555.0 | -457.4 | |
| 1.37 | 2.22 | 1.17 | 1.90 | 18.19 | 235.55 | 52.85 | 291.68 | 0.8171 | -492.9 | -455.9 | |
| 0.00 | 1.88 | 0.00 | 1.61 | 18.44 | 235.51 | 52.80 | 291.99 | 0.8172 | -518.0 | -384.2 | |
| 18.71 | 101.24 | 15.03 | 81.45 | 15.39 | 233.32 | 50.62 | 288.79 | 0.7894 | -881.2 | -191.2 | |
| 1.79 | -4.00 | 1.43 | -4.00 | 15.67 | 232.93 | 50.23 | 289.23 | 0.7860 | -835.3 | 999999 | |
| 5.55 | 7.01 | 4.49 | 5.67 | 16.99 | 233.35 | 50.65 | 290.76 | 0.7932 | -532.4 | -345.1 | |
| 1.28 | 3.50 | 1.02 | 2.78 | 15.89 | 232.67 | 49.96 | 289.57 | 0.7838 | -722.7 | -608.9 | |
| 0.00 | 1.62 | 0.00 | 1.30 | 16.87 | 233.01 | 50.31 | 290.70 | 0.7895 | -670.0 | -617.2 | |
| 0.00 | 1.28 | 0.00 | 0.99 | 15.23 | 231.41 | 48.71 | 289.05 | 0.7693 | -521.0 | -468.9 | |
| 0.00 | 1.37 | 0.00 | 1.07 | 16.64 | 231.78 | 49.08 | 290.74 | 0.7764 | -367.0 | -411.2 | |
| 0.00 | 0.85 | 0.00 | 0.69 | 19.30 | 232.55 | 49.85 | 293.83 | 0.7909 | -425.0 | -374.3 | |
| 0.00 | 0.77 | 0.00 | 0.62 | 19.58 | 232.48 | 49.77 | 294.20 | 0.7909 | -535.0 | -409.4 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 18.78 | 231.43 | 48.73 | 293.53 | 0.7784 | -121.0 | -212.6 | |
| 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. | |