SDO HMI 2014-10-11 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.41 | 0.00 | 8.90 | 14.62 | 56.58 | 9.83 | 314.78 | 0.2251 | 19.4 | 123.8 | |
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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 | 0.88 | 0.00 | 0.46 | 18.25 | 60.97 | 14.21 | 312.42 | 0.3173 | -657.0 | -581.3 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 18.16 | 60.80 | 14.04 | 312.53 | 0.3143 | -850.0 | -677.6 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 17.92 | 60.68 | 13.93 | 312.16 | 0.3103 | -682.0 | -607.9 | |
| 0.00 | 2.45 | 0.00 | 1.26 | 12.77 | 60.04 | 13.29 | 297.87 | 0.2547 | 814.0 | 720.9 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 17.77 | 60.34 | 13.59 | 312.46 | 0.3047 | -926.0 | -705.4 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 16.87 | 59.79 | 13.04 | 311.21 | 0.2883 | -846.0 | -650.2 | |
| 0.00 | 1.40 | 0.00 | 0.72 | 16.46 | 58.93 | 12.18 | 311.94 | 0.2732 | -941.0 | -711.1 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 13.73 | 54.64 | 7.89 | 314.99 | 0.1894 | 770.0 | 607.3 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 13.01 | 54.18 | 7.43 | 313.79 | 0.1753 | 849.0 | 587.3 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.36 | 52.18 | 5.42 | 327.51 | 0.1712 | 799.0 | 711.7 | |
| 0.00 | 2.01 | 0.00 | 1.00 | 11.45 | 50.70 | 3.95 | 324.09 | 0.1156 | 999.0 | 814.5 | |
| 0.00 | 1.66 | 0.00 | 0.83 | 10.81 | 49.01 | 2.26 | 334.63 | 0.0908 | 904.0 | 678.4 | |
| 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. | |