SDO HMI 2014-11-11 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.60 | 0.00 | 10.18 | 19.60 | 341.78 | -19.43 | 48.08 | 0.4246 | 7.8 | -51.9 | |
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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 | 1.12 | 0.00 | 0.60 | 18.83 | 344.00 | -17.21 | 46.04 | 0.3907 | -752.0 | -668.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 16.44 | 344.23 | -16.98 | 50.65 | 0.3638 | -982.0 | -782.7 | |
| 0.00 | 1.55 | 0.00 | 0.82 | 16.25 | 344.18 | -17.03 | 51.14 | 0.3626 | -1017.0 | -793.6 | |
| 0.00 | 2.24 | 0.00 | 1.19 | 16.28 | 343.73 | -17.48 | 51.79 | 0.3686 | -796.0 | -646.1 | |
| 0.00 | 3.45 | 0.00 | 1.85 | 17.00 | 342.81 | -18.40 | 51.57 | 0.3870 | -752.0 | -754.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 24.01 | 341.75 | -19.46 | 40.47 | 0.4708 | 701.0 | 533.8 | |
| 0.00 | 3.36 | 0.00 | 1.87 | 22.65 | 341.44 | -19.77 | 43.03 | 0.4593 | 710.0 | 609.5 | |
| 0.00 | 2.24 | 0.00 | 1.25 | 21.95 | 340.86 | -20.35 | 44.96 | 0.4583 | 834.0 | 702.5 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 25.70 | 337.96 | -23.25 | 42.71 | 0.5264 | 727.0 | 543.1 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 19.41 | 337.13 | -24.08 | 53.75 | 0.4791 | 705.0 | 488.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 19.53 | 336.87 | -24.34 | 53.80 | 0.4833 | 708.0 | 583.3 | |
| 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. | |