SDO HMI 2011-10-18 23:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.23 | 162.06 | 13.06 | 104.40 | -26.88 | 36.71 | 23.58 | 213.91 | 0.6413 | 931.0 | 390.9 | |
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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 |
| 20.23 | 149.08 | 13.06 | 96.31 | -26.88 | 37.10 | 23.97 | 214.37 | 0.6441 | 1079.5 | 371.6 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -27.35 | 33.68 | 20.54 | 210.06 | 0.6245 | 592.0 | 492.8 | |
| 0.00 | 1.57 | 0.00 | 0.99 | -27.41 | 33.48 | 20.34 | 209.76 | 0.6239 | 771.0 | 637.2 | |
| 0.00 | 1.13 | 0.00 | 0.71 | -27.12 | 33.35 | 20.21 | 209.87 | 0.6197 | 642.0 | 471.2 | |
| 0.00 | 2.18 | 0.00 | 1.37 | -27.00 | 32.76 | 19.62 | 209.27 | 0.6142 | 773.0 | 646.0 | |
| 0.00 | 1.31 | 0.00 | 0.82 | -26.78 | 32.57 | 19.44 | 209.24 | 0.6105 | 856.0 | 563.4 | |
| 0.00 | 1.13 | 0.00 | 0.71 | -27.13 | 32.64 | 19.50 | 209.00 | 0.6150 | 612.0 | 501.9 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -27.67 | 32.70 | 19.56 | 208.61 | 0.6217 | 732.0 | 554.7 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -25.05 | 31.09 | 17.96 | 208.92 | 0.5799 | 765.0 | 555.6 | |
| 0.00 | 1.48 | 0.00 | 0.93 | -28.26 | 29.88 | 16.75 | 204.63 | 0.6113 | 829.0 | 697.6 | |
| 0.00 | 1.39 | 0.00 | 0.83 | -25.10 | 28.38 | 15.25 | 205.13 | 0.5629 | 800.0 | 628.4 | |
| 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. | |