SDO HMI 2014-11-03 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.41 | 0.00 | 9.47 | -20.37 | 79.05 | -27.10 | 133.92 | 0.5936 | 713.8 | 588.7 | |
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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 | 2.77 | 0.00 | 1.62 | -20.93 | 85.19 | -20.95 | 141.49 | 0.5385 | 878.0 | 776.1 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -21.07 | 85.11 | -21.04 | 141.54 | 0.5407 | 718.0 | 620.0 | |
| 0.00 | 1.64 | 0.00 | 1.00 | -20.25 | 79.50 | -26.65 | 133.99 | 0.5870 | 644.0 | 526.2 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -20.42 | 79.25 | -26.89 | 133.96 | 0.5911 | 606.0 | 420.3 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -20.67 | 78.67 | -27.48 | 133.69 | 0.5992 | 700.0 | 592.3 | |
| 0.00 | 1.12 | 0.00 | 0.69 | -20.54 | 78.55 | -27.59 | 133.41 | 0.5993 | 726.0 | 654.5 | |
| 0.00 | 2.16 | 0.00 | 1.35 | -20.01 | 76.92 | -29.22 | 131.15 | 0.6115 | 804.0 | 564.7 | |
| 0.00 | 1.30 | 0.00 | 0.82 | -20.35 | 76.63 | -29.51 | 131.33 | 0.6173 | 656.0 | 472.1 | |
| 0.00 | 2.25 | 0.00 | 1.42 | -20.23 | 76.41 | -29.74 | 130.96 | 0.6186 | 680.0 | 573.6 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -19.97 | 76.39 | -29.76 | 130.60 | 0.6167 | 848.0 | 746.5 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -19.77 | 75.70 | -30.45 | 129.72 | 0.6223 | 592.0 | 391.0 | |
| 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. | |