SDO HMI 2014-09-26 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.65 | 18.30 | 2.94 | 20.20 | -14.53 | 185.10 | -60.13 | 110.10 | 0.8954 | -88.7 | -128.7 | |
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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 |
| 0.00 | 1.77 | 0.00 | 1.87 | -14.74 | 186.48 | -58.75 | 110.73 | 0.8859 | 391.0 | 345.2 | |
| 0.97 | 2.56 | 1.01 | 2.65 | -13.55 | 186.92 | -58.31 | 109.57 | 0.8799 | 568.8 | 462.4 | |
| 0.00 | 0.97 | 0.00 | 1.03 | -14.29 | 186.49 | -58.74 | 110.25 | 0.8848 | 125.0 | 213.5 | |
| 0.00 | 0.27 | 0.00 | 0.28 | -13.41 | 186.73 | -58.49 | 109.36 | 0.8810 | 465.0 | 449.7 | |
| 0.00 | 1.33 | 0.00 | 1.38 | -13.27 | 186.55 | -58.68 | 109.15 | 0.8821 | 483.0 | 392.0 | |
| 0.00 | 2.30 | 0.00 | 2.62 | -15.48 | 184.38 | -60.84 | 110.90 | 0.9027 | -540.0 | -462.3 | |
| 0.00 | 2.47 | 0.00 | 2.78 | -14.59 | 184.62 | -60.60 | 110.02 | 0.8992 | -505.0 | -436.9 | |
| 0.00 | 1.68 | 0.00 | 1.92 | -15.27 | 184.23 | -61.00 | 110.64 | 0.9034 | -566.0 | -487.5 | |
| 0.00 | 0.53 | 0.00 | 0.60 | -14.88 | 184.29 | -60.94 | 110.24 | 0.9021 | -529.0 | -473.8 | |
| 0.00 | 0.71 | 0.00 | 0.80 | -14.65 | 184.34 | -60.89 | 110.01 | 0.9014 | -241.0 | -348.4 | |
| 1.68 | 3.71 | 1.93 | 4.27 | -14.58 | 183.85 | -61.37 | 109.79 | 0.9046 | -371.1 | -252.1 | |
| 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. | |