SDO HMI 2011-11-22 04:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.25 | 227.05 | 34.78 | 225.71 | 17.44 | 223.04 | -59.05 | 70.97 | 0.8674 | -470.6 | -98.7 | |
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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 |
| 27.44 | 198.25 | 26.87 | 195.69 | 17.49 | 223.40 | -58.68 | 70.86 | 0.8645 | -824.3 | -165.2 | |
| 2.32 | -1.00 | 2.30 | -1.00 | 17.91 | 222.94 | -59.15 | 70.45 | 0.8689 | -456.1 | 999999 | |
| 1.37 | -1.00 | 1.38 | -1.00 | 18.08 | 222.47 | -59.61 | 70.33 | 0.8729 | -351.2 | 999999 | |
| 1.29 | 1.37 | 1.30 | 1.39 | 16.40 | 222.07 | -60.01 | 72.30 | 0.8742 | -142.7 | -64.0 | |
| 0.00 | 1.54 | 0.00 | 1.61 | 17.89 | 221.25 | -60.83 | 70.73 | 0.8823 | 244.0 | 153.1 | |
| 0.00 | 1.89 | 0.00 | 1.97 | 17.61 | 221.22 | -60.86 | 71.05 | 0.8822 | -233.0 | -86.8 | |
| 0.00 | 1.20 | 0.00 | 1.24 | 16.91 | 221.43 | -60.66 | 71.81 | 0.8799 | 399.0 | 350.3 | |
| 0.00 | 3.77 | 0.00 | 3.96 | 17.33 | 221.00 | -61.09 | 71.40 | 0.8837 | 184.0 | 269.1 | |
| 0.00 | 6.86 | 0.00 | 7.03 | 16.11 | 221.66 | -60.43 | 72.68 | 0.8772 | 270.0 | 308.4 | |
| 0.00 | 2.06 | 0.00 | 2.09 | 15.75 | 221.84 | -60.25 | 73.07 | 0.8754 | 384.0 | 358.1 | |
| 2.83 | 5.23 | 2.93 | 5.42 | 16.53 | 221.31 | -60.78 | 72.25 | 0.8804 | 569.4 | 487.9 | |
| 0.00 | 4.54 | 0.00 | 4.93 | 17.26 | 219.92 | -62.17 | 71.61 | 0.8919 | 594.0 | 535.4 | |
| 0.00 | 0.34 | 0.00 | 0.38 | 16.00 | 219.02 | -63.07 | 73.12 | 0.8974 | 226.0 | 255.8 | |
| 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. | |