SDO HMI 2014-08-06 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.36 | 40.54 | 12.73 | 37.92 | -8.28 | 249.16 | 56.31 | 256.17 | 0.8493 | 130.1 | 72.0 | |
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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 |
| 0.90 | 2.26 | 0.98 | 2.45 | -6.68 | 254.46 | 61.61 | 259.21 | 0.8913 | 451.9 | 340.9 | |
| 0.00 | 0.90 | 0.00 | 0.86 | -7.63 | 249.99 | 57.13 | 257.16 | 0.8559 | 554.0 | 476.9 | |
| 0.00 | 1.08 | 0.00 | 1.03 | -7.81 | 249.97 | 57.12 | 256.94 | 0.8561 | 578.0 | 515.4 | |
| 0.63 | 4.43 | 0.61 | 4.25 | -8.88 | 250.04 | 57.19 | 255.74 | 0.8588 | 431.3 | 370.4 | |
| 7.77 | 12.74 | 7.26 | 11.90 | -6.68 | 249.52 | 56.67 | 258.14 | 0.8500 | 629.7 | 450.6 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -6.99 | 249.46 | 56.61 | 257.77 | 0.8501 | 402.0 | 394.3 | |
| 0.00 | 1.26 | 0.00 | 1.24 | -11.13 | 250.26 | 57.41 | 253.25 | 0.8653 | -366.0 | -300.1 | |
| 1.08 | 10.39 | 1.04 | 9.89 | -9.57 | 249.70 | 56.85 | 254.87 | 0.8572 | -390.2 | -415.3 | |
| 2.98 | -8.00 | 2.84 | -8.00 | -9.71 | 249.51 | 56.66 | 254.66 | 0.8559 | -613.6 | 999999 | |
| 0.00 | 2.62 | 0.00 | 2.32 | -8.36 | 247.12 | 54.27 | 255.57 | 0.8314 | 586.0 | 437.8 | |
| 0.00 | 0.90 | 0.00 | 0.76 | -11.17 | 244.41 | 51.56 | 251.43 | 0.8128 | -152.0 | -216.9 | |
| 0.00 | 0.90 | 0.00 | 0.76 | -10.72 | 244.25 | 51.40 | 251.92 | 0.8100 | -274.0 | -207.7 | |
| 0.00 | 0.63 | 0.00 | 0.52 | -11.18 | 243.42 | 50.57 | 251.08 | 0.8032 | -519.0 | -501.0 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -6.98 | 242.28 | 49.43 | 255.85 | 0.7798 | -534.0 | -436.9 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -8.44 | 240.41 | 47.56 | 253.40 | 0.7640 | -446.0 | -428.5 | |
| 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. | |