SDO HMI 2014-08-13 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.31 | 406.87 | 38.26 | 227.37 | 15.00 | 133.58 | 26.65 | 290.04 | 0.4631 | -894.5 | -319.5 | |
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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 | 0.81 | 0.00 | 0.46 | 16.67 | 135.58 | 28.65 | 292.38 | 0.4987 | 611.0 | 496.1 | |
| 0.00 | 1.44 | 0.00 | 0.81 | 14.22 | 134.64 | 27.71 | 287.97 | 0.4758 | 38.0 | 23.6 | |
| 67.05 | 380.99 | 37.60 | 213.64 | 15.21 | 134.00 | 27.07 | 290.32 | 0.4702 | -1459.6 | -386.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 13.68 | 133.09 | 26.17 | 287.56 | 0.4513 | -770.0 | -590.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 12.59 | 127.41 | 20.48 | 288.21 | 0.3610 | 731.0 | 549.3 | |
| 0.00 | 1.80 | 0.00 | 0.96 | 12.54 | 127.07 | 20.14 | 288.32 | 0.3556 | 908.0 | 725.4 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 12.76 | 127.09 | 20.16 | 288.89 | 0.3568 | 799.0 | 629.9 | |
| 0.00 | 5.14 | 0.00 | 2.72 | 12.49 | 126.90 | 19.97 | 288.29 | 0.3527 | 890.0 | 653.5 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 12.44 | 126.50 | 19.57 | 288.46 | 0.3463 | 796.0 | 677.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 12.11 | 126.34 | 19.41 | 287.64 | 0.3425 | 843.0 | 679.8 | |
| 0.00 | 2.44 | 0.00 | 1.28 | 11.52 | 126.00 | 19.07 | 286.16 | 0.3348 | 833.0 | 728.9 | |
| 0.00 | 1.44 | 0.00 | 0.76 | 9.97 | 125.60 | 18.67 | 281.77 | 0.3235 | 842.0 | 676.2 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 6.83 | 125.06 | 18.13 | 271.96 | 0.3105 | 889.0 | 690.3 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 10.81 | 125.13 | 18.21 | 284.62 | 0.3185 | 900.0 | 672.8 | |
| 1.26 | 3.43 | 0.66 | 1.78 | 10.33 | 124.26 | 17.33 | 283.63 | 0.3029 | 1092.9 | 833.7 | |
| 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. | |