SDO HMI 2011-11-11 23:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.55 | 120.70 | 23.16 | 79.68 | -25.38 | 87.31 | 30.65 | 224.15 | 0.6622 | 78.3 | 184.7 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 1.13 | -25.31 | 91.73 | 35.07 | 227.94 | 0.7021 | -574.0 | -439.9 | |
| 0.00 | 9.90 | 0.00 | 6.67 | -25.10 | 89.52 | 32.87 | 226.48 | 0.6801 | -98.0 | -37.0 | |
| 13.43 | 79.63 | 9.00 | 53.35 | -25.28 | 88.87 | 32.22 | 225.74 | 0.6755 | 946.2 | 402.6 | |
| 4.99 | -3.00 | 3.34 | -3.00 | -25.60 | 88.55 | 31.89 | 225.09 | 0.6751 | 896.7 | 999999 | |
| 3.10 | -3.00 | 2.07 | -3.00 | -25.80 | 88.29 | 31.64 | 224.65 | 0.6744 | 790.5 | 999999 | |
| 0.00 | 0.52 | 0.00 | 0.34 | -25.41 | 87.64 | 30.98 | 224.55 | 0.6652 | 746.0 | 727.2 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -25.43 | 87.45 | 30.80 | 224.36 | 0.6637 | 823.0 | 662.8 | |
| 0.00 | 1.64 | 0.00 | 1.07 | -25.76 | 85.79 | 29.14 | 222.50 | 0.6514 | -747.0 | -566.2 | |
| 0.00 | 1.46 | 0.00 | 0.91 | -24.58 | 82.29 | 25.63 | 220.42 | 0.6090 | -695.0 | -610.6 | |
| 0.00 | 2.84 | 0.00 | 1.77 | -24.61 | 82.04 | 25.38 | 220.13 | 0.6070 | -615.0 | -519.3 | |
| 0.34 | 2.67 | 0.22 | 1.67 | -25.41 | 81.96 | 25.31 | 219.12 | 0.6143 | -679.0 | -523.7 | |
| 2.41 | 12.66 | 1.51 | 7.90 | -25.51 | 81.70 | 25.04 | 218.72 | 0.6129 | -659.8 | -717.1 | |
| 3.53 | 4.82 | 2.19 | 3.00 | -25.03 | 81.52 | 24.86 | 219.08 | 0.6066 | -924.8 | -743.7 | |
| 7.75 | -12.00 | 4.83 | -12.00 | -25.43 | 81.42 | 24.77 | 218.52 | 0.6098 | -863.7 | 999999 | |
| 0.00 | 1.55 | 0.00 | 0.97 | -26.31 | 81.18 | 24.53 | 217.28 | 0.6167 | -739.0 | -526.2 | |
| 0.00 | 0.34 | 0.00 | 0.22 | -26.61 | 81.07 | 24.42 | 216.83 | 0.6188 | -630.0 | -598.8 | |
| 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. | |