SDO HMI 2011-11-26 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.81 | 73.57 | 19.85 | 38.53 | 17.67 | 214.63 | -9.82 | 29.92 | 0.3253 | 465.7 | 273.6 | |
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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 | 1.45 | 0.00 | 0.76 | 17.91 | 218.11 | -6.34 | 20.38 | 0.3030 | 947.0 | 680.5 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 17.45 | 217.97 | -6.48 | 21.37 | 0.2966 | 860.0 | 790.3 | |
| 0.00 | 2.40 | 0.00 | 1.24 | 17.91 | 217.89 | -6.56 | 21.02 | 0.3043 | 675.0 | 642.4 | |
| 0.00 | 4.19 | 0.00 | 2.17 | 17.51 | 217.75 | -6.70 | 21.95 | 0.2989 | 962.0 | 804.2 | |
| 8.30 | 11.21 | 4.30 | 5.81 | 16.83 | 216.75 | -7.70 | 25.85 | 0.2954 | -1012.3 | -540.4 | |
| 1.54 | 5.22 | 0.80 | 2.71 | 16.89 | 216.40 | -8.05 | 26.75 | 0.2989 | -813.8 | -642.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.14 | 215.52 | -8.93 | 23.28 | 0.3679 | 855.0 | 732.5 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 18.24 | 215.61 | -8.83 | 26.82 | 0.3246 | -1077.0 | -891.6 | |
| 0.00 | 2.82 | 0.00 | 1.47 | 16.55 | 215.70 | -8.75 | 29.28 | 0.2995 | -969.0 | -796.6 | |
| 0.00 | 3.17 | 0.00 | 1.66 | 17.34 | 213.58 | -10.86 | 33.34 | 0.3288 | 826.0 | 615.1 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.83 | 213.52 | -10.92 | 32.63 | 0.3360 | 600.0 | 491.1 | |
| 2.82 | 33.62 | 1.49 | 17.73 | 18.05 | 213.22 | -11.22 | 32.96 | 0.3416 | 984.0 | 730.9 | |
| 2.14 | 3.76 | 1.12 | 1.98 | 17.71 | 213.25 | -11.20 | 33.49 | 0.3368 | 1066.4 | 854.4 | |
| 23.01 | -12.00 | 12.14 | -12.00 | 18.04 | 212.81 | -11.63 | 33.90 | 0.3453 | 996.7 | 999999 | |
| 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. | |