SDO HMI 2014-08-19 04:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.29 | 95.98 | 26.88 | 98.23 | -9.44 | 331.30 | -59.06 | 104.78 | 0.8769 | 594.1 | 184.0 | |
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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 |
| 0.00 | 1.35 | 0.00 | 1.18 | -9.35 | 337.14 | -53.22 | 106.33 | 0.8257 | 557.0 | 532.8 | |
| 20.35 | 83.38 | 20.64 | 85.11 | -9.53 | 331.61 | -58.75 | 104.96 | 0.8747 | 774.4 | 179.4 | |
| 0.00 | 0.54 | 0.00 | 0.53 | -6.53 | 331.96 | -58.40 | 101.67 | 0.8661 | 374.0 | 411.2 | |
| 0.00 | 0.99 | 0.00 | 0.98 | -5.73 | 331.63 | -58.73 | 100.69 | 0.8674 | 236.0 | 199.5 | |
| 0.00 | 3.33 | 0.00 | 3.46 | -9.06 | 330.71 | -59.65 | 104.20 | 0.8810 | 419.0 | 383.3 | |
| 5.04 | -2.00 | 5.28 | -2.00 | -9.39 | 330.55 | -59.81 | 104.53 | 0.8828 | 481.9 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.29 | -9.28 | 330.15 | -60.21 | 104.30 | 0.8858 | 189.0 | 183.0 | |
| 0.90 | 2.70 | 0.96 | 2.88 | -9.41 | 330.05 | -60.31 | 104.43 | 0.8868 | 190.2 | 69.8 | |
| 0.00 | 0.99 | 0.00 | 1.07 | -8.74 | 329.29 | -61.07 | 103.50 | 0.8915 | 304.0 | 235.1 | |
| 0.00 | 1.53 | 0.00 | 1.73 | -10.89 | 328.53 | -61.83 | 105.67 | 0.9009 | -420.0 | -367.9 | |
| 0.00 | 0.90 | 0.00 | 1.00 | -9.16 | 328.85 | -61.51 | 103.86 | 0.8956 | 354.0 | 343.4 | |
| 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. | |