SDO HMI 2014-11-29 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.75 | 30.55 | 5.79 | 17.86 | 16.87 | 152.37 | 28.43 | 301.02 | 0.5336 | 188.7 | 63.0 | |
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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 |
| 7.10 | 9.41 | 4.25 | 5.63 | 17.49 | 154.41 | 30.47 | 300.45 | 0.5632 | 899.9 | 643.4 | |
| 1.71 | 3.51 | 1.00 | 2.04 | 15.42 | 152.61 | 28.66 | 298.32 | 0.5274 | 943.7 | 715.6 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 15.18 | 152.43 | 28.49 | 298.03 | 0.5236 | 896.0 | 734.0 | |
| 0.00 | 2.82 | 0.00 | 1.65 | 16.77 | 152.22 | 28.28 | 300.94 | 0.5310 | 725.0 | 574.3 | |
| 0.00 | 1.80 | 0.00 | 1.04 | 16.44 | 151.99 | 28.05 | 300.55 | 0.5259 | 773.0 | 630.1 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 15.89 | 151.87 | 27.93 | 299.70 | 0.5207 | 643.0 | 466.8 | |
| 0.00 | 1.88 | 0.00 | 1.09 | 17.31 | 151.19 | 27.25 | 302.71 | 0.5216 | -735.0 | -590.6 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 16.08 | 150.86 | 26.92 | 300.87 | 0.5089 | -593.0 | -445.6 | |
| 0.00 | 1.80 | 0.00 | 1.03 | 16.51 | 150.55 | 26.60 | 301.90 | 0.5078 | -574.0 | -424.7 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 17.47 | 150.52 | 26.58 | 303.57 | 0.5143 | -825.0 | -761.6 | |
| 0.94 | 2.65 | 0.54 | 1.53 | 17.93 | 150.46 | 26.51 | 304.42 | 0.5170 | -730.7 | -562.3 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 17.13 | 150.33 | 26.39 | 303.17 | 0.5095 | -932.0 | -786.5 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 16.98 | 150.17 | 26.23 | 303.05 | 0.5063 | -772.0 | -602.1 | |
| 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. | |