SDO HMI 2011-11-28 09:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.67 | 0.00 | 13.66 | 17.69 | 214.60 | 14.33 | 320.46 | 0.3712 | 689.8 | 533.7 | |
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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 | 0.56 | 17.98 | 219.13 | 18.85 | 313.23 | 0.4236 | 770.0 | 643.8 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 18.14 | 218.65 | 18.38 | 314.21 | 0.4198 | 1024.0 | 763.7 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 17.83 | 217.77 | 17.49 | 315.01 | 0.4065 | 867.0 | 653.4 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 17.68 | 217.33 | 17.06 | 315.43 | 0.4000 | 901.0 | 755.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 21.14 | 216.89 | 16.61 | 321.98 | 0.4347 | 628.0 | 460.3 | |
| 0.00 | 2.74 | 0.00 | 1.45 | 16.22 | 215.50 | 15.22 | 315.77 | 0.3630 | -850.0 | -706.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.45 | 213.97 | 13.69 | 321.08 | 0.3609 | 772.0 | 703.2 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.46 | 213.46 | 13.18 | 322.11 | 0.3558 | 653.0 | 580.8 | |
| 0.00 | 4.79 | 0.00 | 2.53 | 17.30 | 213.29 | 13.01 | 322.19 | 0.3521 | 902.0 | 713.0 | |
| 0.00 | 1.80 | 0.00 | 0.95 | 17.83 | 213.29 | 13.02 | 323.12 | 0.3588 | 895.0 | 769.2 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 16.54 | 213.01 | 12.73 | 321.33 | 0.3397 | 837.0 | 538.9 | |
| 0.00 | 3.25 | 0.00 | 1.72 | 17.86 | 212.98 | 12.70 | 323.83 | 0.3562 | 516.0 | 705.6 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 17.49 | 212.54 | 12.26 | 324.13 | 0.3472 | 811.0 | 636.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.13 | 212.03 | 11.75 | 329.45 | 0.3778 | 931.0 | 701.5 | |
| 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. | |