SDO HMI 2011-10-14 22:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.85 | 116.03 | 21.24 | 103.14 | -14.65 | 119.14 | 52.69 | 247.89 | 0.8322 | 236.2 | 192.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.88 | 95.93 | 2.60 | 86.92 | -14.01 | 120.01 | 53.56 | 248.96 | 0.8384 | 657.8 | 315.7 | |
| 0.00 | 1.05 | 0.00 | 0.90 | -10.89 | 118.98 | 52.53 | 252.25 | 0.8206 | 472.0 | 410.8 | |
| 17.91 | -1.00 | 16.25 | -1.00 | -14.67 | 119.98 | 53.53 | 248.19 | 0.8400 | 737.8 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.82 | -15.46 | 117.26 | 50.81 | 246.30 | 0.8180 | -292.0 | -222.6 | |
| 0.00 | 1.57 | 0.00 | 1.32 | -16.03 | 116.09 | 49.64 | 245.17 | 0.8092 | -444.0 | -384.9 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -15.45 | 115.66 | 49.20 | 245.67 | 0.8031 | -519.0 | -489.9 | |
| 0.00 | 0.70 | 0.00 | 0.57 | -16.17 | 115.03 | 48.58 | 244.57 | 0.7998 | -570.0 | -529.8 | |
| 0.00 | 1.49 | 0.00 | 1.19 | -14.43 | 114.45 | 48.00 | 246.37 | 0.7878 | -584.0 | -471.9 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -14.31 | 114.41 | 47.96 | 246.51 | 0.7870 | -563.0 | -495.7 | |
| 0.00 | 0.87 | 0.00 | 0.72 | -16.39 | 115.01 | 48.56 | 244.30 | 0.8004 | -330.0 | -389.6 | |
| 0.00 | 1.40 | 0.00 | 1.14 | -16.40 | 114.78 | 48.33 | 244.18 | 0.7983 | -717.0 | -615.3 | |
| 0.00 | 3.67 | 0.00 | 2.97 | -16.24 | 114.31 | 47.85 | 244.17 | 0.7932 | -559.0 | -563.7 | |
| 3.06 | 5.07 | 2.39 | 3.97 | -14.32 | 113.36 | 46.91 | 246.05 | 0.7766 | -607.4 | -436.0 | |
| 0.00 | 2.10 | 0.00 | 1.62 | -14.49 | 112.73 | 46.28 | 245.57 | 0.7709 | -527.0 | -441.0 | |
| 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. | |