SDO HMI 2014-09-28 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.97 | 0.00 | 8.29 | 7.26 | 206.70 | -17.61 | 87.76 | 0.3022 | 586.8 | 517.2 | |
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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 | 0.97 | 0.00 | 0.50 | 6.63 | 208.65 | -15.66 | 89.96 | 0.2693 | -736.0 | -565.1 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 6.58 | 207.93 | -16.38 | 90.07 | 0.2815 | -773.0 | -584.8 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 5.99 | 207.54 | -16.77 | 92.05 | 0.2885 | 876.0 | 675.4 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 5.75 | 207.45 | -16.86 | 92.87 | 0.2903 | 878.0 | 754.8 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 5.98 | 207.29 | -17.03 | 92.02 | 0.2927 | 790.0 | 599.5 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 6.02 | 206.62 | -17.69 | 91.74 | 0.3037 | 703.0 | 605.8 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 6.95 | 206.56 | -17.76 | 88.67 | 0.3042 | 850.0 | 681.8 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 7.19 | 206.48 | -17.83 | 87.88 | 0.3053 | 735.0 | 532.4 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 8.30 | 206.34 | -17.97 | 84.27 | 0.3082 | 936.0 | 761.6 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 8.96 | 206.28 | -18.04 | 82.15 | 0.3101 | 918.0 | 713.8 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 6.79 | 206.28 | -18.04 | 89.17 | 0.3089 | 755.0 | 682.4 | |
| 0.00 | 2.47 | 0.00 | 1.29 | 8.33 | 205.73 | -18.58 | 84.26 | 0.3183 | 852.0 | 683.9 | |
| 0.00 | 1.59 | 0.00 | 0.83 | 8.51 | 205.66 | -18.65 | 83.71 | 0.3197 | 845.0 | 708.1 | |
| 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. | |