SDO HMI 2014-01-10 09:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.47 | 0.00 | 9.56 | -17.06 | 69.95 | 3.91 | 197.09 | 0.2944 | -488.6 | -446.0 | |
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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 | 1.70 | 0.00 | 0.88 | -13.11 | 80.90 | 14.87 | 237.45 | 0.2978 | -861.0 | -642.8 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -12.78 | 80.73 | 14.69 | 238.12 | 0.2926 | -962.0 | -831.1 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -12.64 | 80.59 | 14.56 | 238.34 | 0.2895 | -944.0 | -771.9 | |
| 0.00 | 1.70 | 0.00 | 0.88 | -16.04 | 77.38 | 11.35 | 222.17 | 0.2830 | -829.0 | -605.8 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -15.42 | 75.86 | 9.82 | 219.72 | 0.2586 | 856.0 | 664.5 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -25.18 | 75.50 | 9.47 | 202.40 | 0.3923 | 802.0 | 583.0 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -13.98 | 72.79 | 6.75 | 213.45 | 0.2079 | -774.0 | -569.9 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -21.92 | 72.26 | 6.22 | 198.14 | 0.3245 | 682.0 | 576.9 | |
| 0.00 | 1.45 | 0.00 | 0.73 | -16.52 | 63.66 | -2.38 | 169.55 | 0.2204 | -941.0 | -736.0 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -18.39 | 61.36 | -4.68 | 162.65 | 0.2606 | -845.0 | -735.0 | |
| 0.00 | 2.04 | 0.00 | 1.05 | -15.77 | 54.55 | -11.48 | 136.84 | 0.2813 | -930.0 | -825.2 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -24.29 | 53.49 | -12.54 | 150.32 | 0.4015 | -770.0 | -691.2 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -25.11 | 53.01 | -13.03 | 150.50 | 0.4162 | -836.0 | -641.3 | |
| 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. | |