SDO HMI 2011-11-25 04:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.29 | 63.03 | 26.46 | 57.52 | 16.36 | 298.61 | 56.07 | 288.51 | 0.8411 | -142.6 | -131.4 | |
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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 | 0.77 | 0.00 | 0.82 | 14.57 | 304.12 | 61.57 | 285.62 | 0.8858 | 315.0 | 296.9 | |
| 13.10 | 28.86 | 12.47 | 27.47 | 16.16 | 300.27 | 57.73 | 287.96 | 0.8558 | -645.0 | -260.0 | |
| 0.00 | 2.74 | 0.00 | 2.60 | 16.72 | 300.07 | 57.53 | 288.64 | 0.8548 | -411.0 | -335.4 | |
| 2.23 | 3.34 | 2.05 | 3.08 | 15.45 | 299.22 | 56.67 | 287.30 | 0.8456 | -476.6 | -379.7 | |
| 2.57 | 4.11 | 2.27 | 3.63 | 15.36 | 297.48 | 54.93 | 287.49 | 0.8297 | 203.6 | -70.9 | |
| 0.00 | 3.08 | 0.00 | 2.75 | 16.19 | 297.76 | 55.21 | 288.42 | 0.8335 | 183.0 | 139.0 | |
| 0.34 | 1.37 | 0.30 | 1.20 | 15.53 | 297.11 | 54.57 | 287.75 | 0.8265 | -608.5 | -473.1 | |
| 0.00 | 0.77 | 0.00 | 0.67 | 15.99 | 296.71 | 54.17 | 288.39 | 0.8235 | -481.0 | -523.8 | |
| 0.00 | 0.77 | 0.00 | 0.67 | 15.87 | 296.66 | 54.12 | 288.25 | 0.8229 | -429.0 | -346.2 | |
| 0.00 | 0.60 | 0.00 | 0.53 | 17.00 | 297.03 | 54.48 | 289.54 | 0.8281 | 198.0 | 254.1 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 16.19 | 296.42 | 53.88 | 288.68 | 0.8211 | -669.0 | -503.7 | |
| 0.00 | 0.94 | 0.00 | 0.80 | 17.04 | 295.46 | 52.92 | 289.90 | 0.8134 | 84.0 | 167.8 | |
| 7.88 | 14.82 | 6.70 | 12.56 | 17.56 | 295.52 | 52.98 | 290.52 | 0.8150 | 582.3 | 522.5 | |
| 3.17 | -13.00 | 2.67 | -13.00 | 17.26 | 295.14 | 52.60 | 290.24 | 0.8108 | 599.6 | 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. | |