SDO HMI 2011-11-22 21:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.55 | 270.48 | 30.32 | 214.59 | 17.29 | 222.93 | -49.82 | 69.27 | 0.7822 | -569.6 | -171.7 | |
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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 |
| 33.76 | 224.89 | 26.47 | 177.21 | 17.41 | 223.40 | -49.35 | 69.01 | 0.7777 | -1034.6 | -295.3 | |
| 3.34 | -1.00 | 2.68 | -1.00 | 17.97 | 222.36 | -50.39 | 68.57 | 0.7895 | -532.1 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.55 | 17.72 | 222.11 | -50.64 | 68.95 | 0.7914 | -221.0 | -168.8 | |
| 0.00 | 1.88 | 0.00 | 1.53 | 17.93 | 221.93 | -50.82 | 68.73 | 0.7937 | -234.0 | -123.3 | |
| 1.11 | 6.00 | 0.89 | 4.78 | 15.51 | 222.24 | -50.51 | 71.68 | 0.7857 | 610.2 | 361.1 | |
| 0.00 | 0.69 | 0.00 | 0.55 | 15.87 | 221.97 | -50.78 | 71.29 | 0.7891 | 803.0 | 711.5 | |
| 0.34 | 24.42 | 0.28 | 19.79 | 16.29 | 221.67 | -51.08 | 70.83 | 0.7929 | 47.5 | 315.8 | |
| 0.00 | 0.94 | 0.00 | 0.78 | 16.09 | 220.85 | -51.90 | 71.26 | 0.8008 | 634.0 | 577.2 | |
| 0.00 | 1.20 | 0.00 | 1.00 | 16.38 | 220.38 | -52.37 | 70.99 | 0.8059 | 411.0 | 449.7 | |
| 0.00 | 2.23 | 0.00 | 1.88 | 17.26 | 219.93 | -52.82 | 70.01 | 0.8119 | 670.0 | 615.0 | |
| 0.00 | 0.69 | 0.00 | 0.58 | 17.28 | 219.51 | -53.24 | 70.07 | 0.8160 | 453.0 | 410.8 | |
| 0.00 | 1.88 | 0.00 | 1.62 | 17.33 | 219.01 | -53.74 | 70.12 | 0.8207 | 633.0 | 512.6 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 16.93 | 218.97 | -53.78 | 70.61 | 0.8204 | 383.0 | 330.3 | |
| 0.00 | 3.17 | 0.00 | 2.75 | 17.32 | 218.70 | -54.05 | 70.19 | 0.8236 | 287.0 | 319.3 | |
| 0.00 | 0.94 | 0.00 | 0.83 | 17.50 | 218.35 | -54.40 | 70.05 | 0.8271 | 283.0 | 193.0 | |
| 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. | |