SDO HMI 2011-11-01 22:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.05 | 457.42 | 168.28 | 1650.50 | 18.99 | 108.84 | -80.22 | 71.46 | 0.9831 | 84.5 | 101.7 | |
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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 |
| 2.08 | 7.44 | 6.01 | 21.41 | 22.19 | 108.00 | -81.06 | 68.21 | 0.9859 | -481.4 | -345.2 | |
| 5.97 | 27.69 | 26.98 | 136.85 | 21.71 | 104.15 | -84.91 | 68.60 | 0.9944 | 452.6 | 497.4 | |
| 5.45 | 416.23 | 13.47 | 1468.40 | 19.39 | 109.86 | -79.20 | 71.07 | 0.9804 | -445.8 | 78.6 | |
| 11.85 | -3.00 | 26.79 | -3.00 | 18.66 | 110.99 | -78.07 | 71.83 | 0.9766 | -580.6 | 999999 | |
| 0.95 | -3.00 | 2.32 | -3.00 | 18.93 | 110.03 | -79.03 | 71.54 | 0.9799 | -219.0 | 999999 | |
| 14.88 | -3.00 | 38.11 | -3.00 | 19.05 | 109.46 | -79.60 | 71.42 | 0.9817 | 349.1 | 999999 | |
| 1.64 | -3.00 | 4.05 | -3.00 | 18.64 | 109.88 | -79.18 | 71.84 | 0.9804 | -263.8 | 999999 | |
| 2.25 | -2.00 | 12.37 | -2.00 | 20.61 | 103.01 | -86.05 | 69.67 | 0.9963 | 536.8 | 999999 | |
| 2.51 | -3.00 | 7.02 | -3.00 | 18.32 | 108.47 | -80.58 | 72.15 | 0.9847 | -126.1 | 999999 | |
| 9.00 | -3.00 | 26.89 | -3.00 | 18.36 | 107.77 | -81.29 | 72.09 | 0.9867 | 358.2 | 999999 | |
| 1.47 | -3.00 | 4.27 | -3.00 | 17.97 | 107.99 | -81.07 | 72.49 | 0.9861 | -144.3 | 999999 | |
| 0.00 | 1.73 | 0.00 | 6.71 | 17.27 | 105.29 | -83.77 | 73.11 | 0.9926 | 72.0 | 49.7 | |
| 0.00 | 4.33 | 0.00 | 17.13 | 16.86 | 105.28 | -83.77 | 73.52 | 0.9927 | 65.0 | 88.4 | |
| 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. | |