SDO HMI 2011-11-29 14:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.86 | 132.53 | 24.89 | 103.34 | 15.83 | 233.36 | 49.00 | 289.73 | 0.7737 | -753.8 | -257.7 | |
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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 | 1.03 | 0.00 | 0.83 | 16.56 | 235.24 | 50.88 | 290.17 | 0.7946 | -447.0 | -368.2 | |
| 1.11 | 1.20 | 0.91 | 0.98 | 17.82 | 235.58 | 51.22 | 291.63 | 0.8007 | -366.9 | -384.0 | |
| 0.00 | 1.28 | 0.00 | 1.05 | 17.60 | 235.49 | 51.14 | 291.39 | 0.7994 | -532.0 | -477.1 | |
| 1.79 | 5.21 | 1.47 | 4.29 | 18.13 | 235.46 | 51.10 | 292.05 | 0.8002 | -594.4 | -440.5 | |
| 19.57 | 105.11 | 15.20 | 81.77 | 15.42 | 233.36 | 49.00 | 289.21 | 0.7728 | -931.4 | -199.5 | |
| 2.56 | -5.00 | 1.98 | -5.00 | 15.70 | 232.94 | 48.58 | 289.68 | 0.7690 | -818.4 | 999999 | |
| 5.55 | 7.52 | 4.34 | 5.87 | 16.89 | 233.29 | 48.93 | 291.09 | 0.7755 | -562.8 | -436.0 | |
| 1.28 | 2.39 | 0.99 | 1.85 | 16.68 | 232.98 | 48.62 | 290.91 | 0.7718 | -684.1 | -656.8 | |
| 0.00 | 3.16 | 0.00 | 2.43 | 15.86 | 232.71 | 48.35 | 289.94 | 0.7669 | -779.0 | -715.0 | |
| 0.00 | 1.11 | 0.00 | 0.83 | 15.23 | 231.55 | 47.19 | 289.44 | 0.7530 | -728.0 | -590.1 | |
| 0.00 | 0.85 | 0.00 | 0.66 | 19.58 | 232.41 | 48.05 | 294.73 | 0.7738 | -399.0 | -414.8 | |
| 0.00 | 0.60 | 0.00 | 0.46 | 19.36 | 232.09 | 47.73 | 294.56 | 0.7699 | -556.0 | -527.3 | |
| 0.00 | 1.79 | 0.00 | 1.39 | 19.52 | 232.01 | 47.65 | 294.79 | 0.7696 | -605.0 | -560.1 | |
| 0.00 | 1.28 | 0.00 | 0.93 | 15.99 | 229.42 | 45.06 | 291.07 | 0.7316 | -641.0 | -536.3 | |
| 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. | |