SDO HMI 2014-05-19 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.74 | 24.02 | 4.27 | 13.17 | 9.65 | 180.14 | 22.46 | 298.40 | 0.4296 | -108.2 | -96.3 | |
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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 | 0.54 | 0.00 | 0.31 | 12.23 | 184.41 | 26.73 | 299.05 | 0.5049 | 392.0 | 450.2 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 7.46 | 183.07 | 25.39 | 291.00 | 0.4573 | -635.0 | -543.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | 11.62 | 181.81 | 24.13 | 300.38 | 0.4660 | -666.0 | -515.2 | |
| 3.24 | 12.32 | 1.79 | 6.81 | 9.13 | 181.43 | 23.75 | 295.81 | 0.4435 | -942.4 | -729.2 | |
| 4.50 | -4.00 | 2.48 | -4.00 | 9.41 | 181.35 | 23.67 | 296.46 | 0.4442 | -995.4 | 999999 | |
| 0.00 | 1.80 | 0.00 | 0.99 | 9.50 | 181.09 | 23.41 | 296.89 | 0.4411 | -917.0 | -810.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 6.81 | 178.25 | 20.57 | 293.71 | 0.3826 | 696.0 | 616.8 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 10.33 | 178.43 | 20.74 | 301.51 | 0.4104 | 559.0 | 435.9 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 11.26 | 177.87 | 20.18 | 304.14 | 0.4106 | 787.0 | 621.3 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 9.93 | 176.14 | 18.46 | 303.61 | 0.3760 | 628.0 | 548.0 | |
| 0.00 | 2.25 | 0.00 | 1.20 | 9.81 | 175.94 | 18.26 | 303.60 | 0.3722 | 878.0 | 695.3 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 11.56 | 174.11 | 16.42 | 310.35 | 0.3650 | 890.0 | 679.8 | |
| 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. | |