SDO HMI 2011-11-24 19:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.76 | 38.07 | 18.08 | 52.84 | 18.77 | 315.91 | 68.42 | 289.49 | 0.9346 | -239.1 | -118.8 | |
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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 |
| 1.97 | 2.57 | 2.91 | 3.79 | 17.70 | 317.44 | 69.95 | 288.19 | 0.9435 | -229.2 | -164.6 | |
| 0.00 | 0.68 | 0.00 | 0.99 | 17.55 | 317.13 | 69.64 | 288.06 | 0.9417 | -541.0 | -469.5 | |
| 5.22 | 15.06 | 7.94 | 22.97 | 18.81 | 318.00 | 70.51 | 289.31 | 0.9470 | -551.4 | -283.0 | |
| 0.00 | 2.65 | 0.00 | 3.82 | 17.78 | 316.87 | 69.38 | 288.32 | 0.9403 | -448.0 | -444.9 | |
| 3.60 | 4.62 | 4.89 | 6.29 | 19.31 | 315.51 | 68.02 | 290.08 | 0.9333 | -526.8 | -436.8 | |
| 0.00 | 0.94 | 0.00 | 1.21 | 17.79 | 314.11 | 66.62 | 288.59 | 0.9238 | 367.0 | 273.3 | |
| 0.00 | 0.94 | 0.00 | 1.20 | 19.10 | 313.94 | 66.45 | 290.02 | 0.9236 | -445.0 | -440.1 | |
| 0.00 | 2.48 | 0.00 | 3.00 | 18.61 | 312.49 | 64.99 | 289.66 | 0.9138 | 336.0 | 250.6 | |
| 1.97 | 5.56 | 2.34 | 6.63 | 19.53 | 311.91 | 64.41 | 290.74 | 0.9107 | 489.0 | 390.4 | |
| 0.00 | 0.94 | 0.00 | 1.09 | 18.67 | 311.29 | 63.80 | 289.88 | 0.9057 | 212.0 | 144.5 | |
| 0.00 | 0.86 | 0.00 | 0.97 | 19.22 | 310.61 | 63.11 | 290.57 | 0.9014 | 409.0 | 395.5 | |
| 0.00 | 0.77 | 0.00 | 0.88 | 19.65 | 310.91 | 63.42 | 291.00 | 0.9040 | 351.0 | 314.3 | |
| 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. | |