SDO HMI 2011-08-07 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.11 | 71.43 | 14.09 | 38.48 | -16.63 | 242.80 | -2.17 | 174.91 | 0.3932 | -230.4 | 149.6 | |
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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 | 0.81 | -14.72 | 246.41 | 1.44 | 183.90 | 0.3598 | 956.0 | 752.4 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -15.83 | 245.76 | 0.79 | 182.01 | 0.3773 | 796.0 | 706.7 | |
| 0.00 | 3.25 | 0.00 | 1.73 | -15.08 | 245.47 | 0.50 | 181.33 | 0.3649 | 926.0 | 761.3 | |
| 3.25 | 11.65 | 1.73 | 6.22 | -15.44 | 245.31 | 0.34 | 180.90 | 0.3707 | 970.6 | 522.2 | |
| 5.24 | 24.39 | 2.82 | 13.12 | -16.62 | 244.17 | -0.80 | 178.04 | 0.3901 | 914.3 | 310.8 | |
| 2.44 | -5.00 | 1.31 | -5.00 | -16.82 | 243.70 | -1.27 | 176.89 | 0.3936 | -728.2 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -16.36 | 242.88 | -2.09 | 174.78 | 0.3872 | 914.0 | 656.1 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -17.09 | 242.74 | -2.23 | 174.63 | 0.3991 | -620.0 | -568.5 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.07 | 240.65 | -4.32 | 170.54 | 0.4347 | -793.0 | -547.7 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -16.94 | 240.67 | -4.30 | 169.67 | 0.4012 | -991.0 | -819.8 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -17.14 | 240.57 | -4.40 | 169.52 | 0.4046 | -939.0 | -720.2 | |
| 1.45 | 3.07 | 0.78 | 1.66 | -16.94 | 240.20 | -4.77 | 168.55 | 0.4027 | -1027.3 | -879.3 | |
| 13.73 | 18.06 | 7.45 | 9.80 | -17.31 | 239.99 | -4.98 | 168.27 | 0.4090 | -981.3 | -629.6 | |
| 0.00 | 1.90 | 0.00 | 1.04 | -18.60 | 237.70 | -7.27 | 164.03 | 0.4376 | -760.0 | -561.1 | |
| 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. | |