SDO HMI 2014-08-22 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.14 | 133.28 | 13.41 | 88.07 | 16.52 | 28.01 | 41.14 | 287.24 | 0.6623 | -491.2 | -269.4 | |
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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 |
| 18.16 | 115.01 | 12.10 | 76.69 | 16.40 | 28.71 | 41.84 | 286.86 | 0.6709 | -1060.1 | -320.0 | |
| 1.98 | -1.00 | 1.31 | -1.00 | 16.37 | 28.28 | 41.41 | 286.90 | 0.6655 | -966.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 17.65 | 26.61 | 39.73 | 289.23 | 0.6474 | -689.0 | -629.3 | |
| 0.00 | 2.43 | 0.00 | 1.55 | 14.15 | 25.79 | 38.91 | 283.97 | 0.6299 | -630.0 | -471.3 | |
| 0.00 | 1.80 | 0.00 | 1.17 | 17.93 | 26.64 | 39.77 | 289.64 | 0.6485 | -591.0 | -526.8 | |
| 0.00 | 1.17 | 0.00 | 0.75 | 16.98 | 26.02 | 39.15 | 288.35 | 0.6384 | -745.0 | -647.8 | |
| 0.00 | 1.08 | 0.00 | 0.69 | 17.48 | 25.99 | 39.11 | 289.13 | 0.6392 | -412.0 | -406.2 | |
| 0.00 | 1.53 | 0.00 | 0.97 | 16.93 | 24.96 | 38.08 | 288.56 | 0.6246 | -778.0 | -580.5 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 17.06 | 21.74 | 34.87 | 289.78 | 0.5830 | 673.0 | 559.7 | |
| 0.00 | 1.53 | 0.00 | 0.93 | 17.44 | 21.24 | 34.37 | 290.60 | 0.5775 | 685.0 | 622.7 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 19.11 | 21.51 | 34.63 | 293.28 | 0.5868 | 517.0 | 408.3 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 19.40 | 21.27 | 34.39 | 293.87 | 0.5848 | 645.0 | 491.6 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 18.25 | 20.77 | 33.89 | 292.16 | 0.5740 | 827.0 | 615.0 | |
| 0.00 | 1.89 | 0.00 | 1.14 | 18.89 | 20.53 | 33.65 | 293.34 | 0.5732 | 785.0 | 634.0 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 17.05 | 19.64 | 32.76 | 290.55 | 0.5546 | 832.0 | 722.9 | |
| 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. | |